HEIC: Terzan 5: Commotion in a Crowded Cluster

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HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by bystander » Mon May 23, 2011 3:25 pm

Terzan 5: Commotion in a Crowded Cluster
ESA/HEIC Hubble Picture of the Week | 2011 May 23

Deep within the Milky Way lies the ancient globular cluster Terzan 5. This NASA/ESA Hubble Space Telescope image shows the cluster in wonderful detail, but it is the chaotic motions of its stars that make it particularly interesting to astronomers.

Terzan 5 has an exceptionally dense core. As a result, it is thought to have one of the highest stellar collision rates for a globular cluster. And packed in at such close quarters, many stars are pushed so close together that they form tight binary systems.

Interestingly, studies of individual stars within the cluster reveal that they can be split into two age groups: 6 and 12 billion years old. Some astronomers have hypothesised that the younger crowd may have been stripped away from a dwarf galaxy.

This picture was created from images taken with the Wide Field Channel of Hubble’s Advanced Camera for Surveys. Images through a yellow/red filter (F606W, coloured blue) have been combined with those through a near-infrared filter (F814W, coloured red) to create this composite picture. The total exposure times per filter were 340 s and 360 s, respectively and the field of view is 3.1 x 1.4 arcminutes.

Credit: NASA/ESA/Hubble

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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by owlice » Mon May 23, 2011 3:42 pm

What a pretty cluster!
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by neufer » Mon May 23, 2011 4:51 pm

http://en.wikipedia.org/wiki/PSR_J1748-2446ad wrote:
<<PSR J1748-2446ad is the fastest-spinning pulsar known, at 716 Hz. (The previous record was held by PSR B1937+21, discovered in 1982, spinning at 642 Hz.) This pulsar was discovered by Jason W. T. Hessels of McGill University on November 10, 2004 and confirmed on January 8, 2005. Hessels speculates that gravitational radiation from the pulsar might be detectable by LIGO.

Scientists' calculation assume that the neutron star contains slightly less than two times the mass of the Sun, which is approximately the same for all neutron stars. Its radius is constrained to be less than 16 km. At its equator it is spinning at approximately 24% of the speed of light, or over 70,000 km per second.

The pulsar is located in a globular cluster of stars called Terzan 5, located approximately 18,000 light-years from Earth in the constellation Sagittarius. It is part of a binary system and undergoes regular eclipses with an eclipse fraction of about 40%. Its orbit is highly circular with a 26 hour period and a radius of 4–5 earth radii. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii. Hessels states that the companion may be a "bloated main-sequence star, possibly still filling its Roche Lobe".>>
Art (a bloated main-sequence poster, possibly filling his Roche Lobe) Neuendorffer
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by DEB » Thu Jun 02, 2011 3:23 pm

Something is not right here...

"Its orbit is highly circular with a 26 hour period and a radius of 4–5 earth radii. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii."

In lay terms, we have two objects orbiting 20,000 miles apart, one of which is 6,000,000 miles across. The pulsar is orbiting DEEP inside the "bloated main-sequence star".

The Wikipedia article referenced does not include "and a radius of 4-5 earth radii". I assume the orbital radius has to be at least 6 SOLAR radii, just to be above the surface of the star.

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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by neufer » Thu Jun 02, 2011 4:12 pm

DEB wrote:Something is not right here...

"Its orbit is highly circular with a 26 hour period and a radius of 4–5 earth radii. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii."

In lay terms, we have two objects orbiting 20,000 miles apart, one of which is 6,000,000 miles across. The pulsar is orbiting DEEP inside the "bloated main-sequence star".

The Wikipedia article referenced does not include "and a radius of 4-5 earth radii". I assume the orbital radius has to be at least 6 SOLAR radii, just to be above the surface of the star.
The 4–5 earth radii & 5–6 solar radii correspond to the sizes of the two stars NOT their separation.

The 26 hour period corresponds to an orbital separation of ~3 million miles.

The sun is 865,000 miles in diameter so 5–6 solar radii ~ 2.4 million miles.
http://hera.ph1.uni-koeln.de/~heintzma/PSR1/NRAO_3C58.htm wrote: <<Terzan 5ad (formally known as PSR J1748–2446ad) belongs to a class known as millisecond pulsars. These bizarre objects are neutron stars (the ultradense cores of massive stars) that take only a few thousandths of a second to complete one rotation. Most known pulsars have rotation periods ranging from a few times per second to a few times per minute, and these rates slow down over time as pulsars emit winds of gas, which act to brake the object's spin. Millisecond pulsars, on the other hard, are literally "spun up" as they accrete material from a binary companion star. This matter falls onto the pulsar's equator, transferring some of its orbital energy to the pulsar's rotation rate.

Using the 100-meter Green Bank Telescope in West Virginia, a team led by Scott Ransom (National Radio Astronomy Observatory) targeted the globular cluster Terzan 5 for millisecond pulsars. This cluster is about 28,000 light-years from Earth in the constellation Sagittarius. Ransom and his colleagues refer to this crowded star cluster as a "millsecond pulsar factory" because conditions are ripe for their formation.

"The cores of globular clusters are extremely dense, so stars can have collisions and interactions," says Ransom. "An ancient neutron star can encounter a binary system. The neutron star picks up a new companion in the exchange — an example of partner swapping." It's these interactions that can produce the binary systems that can spin-up pulsars to millisecond speeds.

Last year, Ransom and his colleagues announced 21 new millisecond pulsars in Terzan 5, adding to the three previously known within this globular. But today, at the American Astronomical Society meeting in Washington, DC, Ransom announced 9 new ones giving Terzan 5 a grand total of 33 pulsars. And by using a specially designed signal processor known as the Pulsar Spigot system, they found that Terzan 5ad spins once every 1.39 milliseconds, or 716 times per second. The previous record holder, which by coincidence was also the first millisecond pulsar discovered, spins "only" 642 times per second.

"We believe that the matter in neutron stars is denser than an atomic nucleus, but it is unclear by how much. Our observations of such a rapidly rotating star set a hard upper limit on its size, and hence on how dense the star can be," adds team member Jason Hessels. The pulsar can't be more than 30 kilometers (20 miles) across, otherwise the ultrafast spin would begin to break it apart.>>
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by DEB » Thu Jun 02, 2011 4:58 pm

Sorry to be picky, I'm just trying to get the facts straight.

"The 4–5 earth radii & 5–6 solar radii correspond to the sizes of the two stars NOT their separation. "
The pulsar has a radius of ~16km (from your earlier posting), the star has a radius of 5-6 solar radii. The orbit has a radius of ~6 solar radii.
Nothing in this system is 4-5 earth radii.

"The 26 hour period corresponds to an orbital separation of ~3 million miles."
Cool. That's damn close to my guess of "at least 6 SOLAR radii, ie 865k*3 = 2.595M miles

"The sun is 865,000 miles in diameter so 5–6 solar radii ~ 2.4 million miles."
That's 2.4 million miles in radius, or 4.8 million miles across. I was using a round figure of 1M miles for the sun's diameter and came up with a figure of 6M miles across. I stand corrected.

It's an extremely cool system, it gets my vote for an APOD. Thanks for sharing.

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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by owlice » Thu Jun 02, 2011 5:09 pm

DEB, you might want to mention on the poll thread why you think this image would make a good APOD; you may be able to influence future voters into voting for it!
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by bystander » Thu Jun 02, 2011 5:44 pm

neufer wrote:The 4–5 earth radii & 5–6 solar radii correspond to the sizes of the two stars NOT their separation.
A neutron star of ~ 2 M with a radius of 4-5 R? Possibly, but the stated radius of < 16 km is more like 2-3 R. Your wiki quote was awkwardly worded and it seemed the 4-5 R did refer to the orbital radius of the neutron star. I'm not sure where you got that anyway, as DEB noted, it isn't included in wiki any more. The first I found it in the wiki history was before the Feb 2010 edit.
Wiki [i](current)[/i] wrote:The pulsar is located in a globular cluster of stars called Terzan 5, located approximately 18,000 light-years from Earth in the constellation Sagittarius. It is part of a binary system and undergoes regular eclipses with an eclipse fraction of about 40%. Its orbit is highly circular with a 26 hour period. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii. Hessels states that the companion may be a "bloated main-sequence star, possibly still filling its Roche Lobe".
Wiki [i](prior to 11 Feb 2010)[/i] wrote:The pulsar is located in a globular cluster of stars called Terzan 5, located approximately 18,000 light-years from Earth in the constellation Sagittarius. It is part of a binary system and undergoes regular eclipses with an eclipse fraction of about 40%. Its orbit is highly circular with a 26 hour period and a radius of 4–5 earth radii. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii. Hessels states that the companion may be a "bloated main-sequence star, possibly still filling its Roche Lobe".
I'm not sure why they say the neutron star is orbiting the other. With a mass of only ~ 0.14 M, it seems it would be more proper to say this is the orbiting body even if it is "bloated" to 5–6 R.
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by neufer » Thu Jun 02, 2011 6:18 pm

bystander wrote:
neufer wrote:
The 4–5 earth radii & 5–6 solar radii correspond to the sizes of the two stars NOT their separation.
A neutron star of ~ 2 M with a radius of 4-5 R? I don't think so. The way I read your wiki quote the 4-5 R did refer to the orbital radius of the neutron star. I'm not sure where you got that anyway, as DEB noted, it isn't included in wiki any more. The first I found it in the wiki history was before the Feb 2010 edit.
As in Sat May 02, 2009 2:37 pm :?:

I have lost 10 lbs since 2009 so my bloated joke is also somewhat obsolete;
but I just say to myself: "Write it down, it's a good Roche Lobe joke!"
http://en.wikipedia.org/wiki/Hal_Roach_%28comedian%29 wrote:
<<Hal Roach (born November 4, 1927 in Waterford), is a prominent Irish comedian. He has spent over 60 years in show business, and was featured in the Guinness Book of Records for the longest-running engagement of a comedian at the same venue: 26 years at Jury's Irish Cabaret, Dublin. Born John Roach, he initially toured with an illusionist and specialised in magic, but later moved to comedy.
  • A typical Hal Roach joke is as follows:
    "He told me that I have a cult following, at least I think that's what he said".

    Another- "There is a man sitting in the middle of the road casting his fishing line...
    now none of us is perfect, but c'mon! So I asked him, "How many have you caught today?"
    He said, "You're the ninth."
Perhaps his most famous catchphrase is "Write it down, it's a good one!".>>
bystander wrote:
Wiki [i](current)[/i] wrote:The pulsar is located in a globular cluster of stars called Terzan 5, located approximately 18,000 light-years from Earth in the constellation Sagittarius. It is part of a binary system and undergoes regular eclipses with an eclipse fraction of about 40%. Its orbit is highly circular with a 26 hour period. The other object is about 0.14 solar masses, with a radius of 5–6 solar radii. Hessels states that the companion may be a "bloated main-sequence star, possibly still filling its Roche Lobe".
I'm not sure why they say the neutron star is orbiting the other. With a mass of ~ 0.14 M, it seems it would be more proper to say this is the orbiting body even if it is "bloated" to 5–6 R.
Well... they ARE actually observing the pulsar orbiting the mutual center of gravity by using the modulation in the pulse frequency.

Everything else is secondary and somewhat speculative.
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by bystander » Thu Jun 02, 2011 6:27 pm

neufer wrote:Well... they ARE actually observing the pulsar orbiting the mutual center of gravity by using the modulation in the pulse frequency.

Everything else is secondary and somewhat speculative.
So the 4-5 R could be the orbital radius around the center of mass???

BTW: I edited my OP before you responded to reflect earth radius instead of solar radius.
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by neufer » Thu Jun 02, 2011 10:55 pm

bystander wrote:
neufer wrote:Well... they ARE actually observing the pulsar orbiting the mutual center of gravity by using the modulation in the pulse frequency.

Everything else is secondary and somewhat speculative.
So the 4-5 R could be the orbital radius around the center of mass???
No.

The orbital radius around the center of mass corresponds to the amplitude of periodic delay in pulses (every 26 hours)
which must be something on the order of ±1.6 light seconds or ~300,000 miles = 75 R
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Re: HEIC: Terzan 5: Commotion in a Crowded Cluster

Post by bystander » Fri Jun 24, 2011 5:55 pm

Spectacular and sparkling, but what is it?
Discover Blogs | Bad Astronomy | 2011 June 01
Globular clusters are among the most spectacular of objects in the entire night sky. Compact balls of hundreds of thousands of stars, well over a hundred orbit our galaxy at various distances. When viewed by Hubble, the result is nothing less than jaw-dropping: [Click to embiggen, and please do; I had to crop the image to get it to fit and the full-size version is even more spectacular!]

This view of Terzan 5, as it’s called, is gorgeous! The thing is… Terzan 5 may not really be a globular cluster. Sure, it’s a cluster, and it’s globular, but it may not be what we usually think of as a globular cluster.

When I read the press release for the picture, the name Terzan 5 looked familiar. So I searched my blog, and found I’ve written about this object before. That post was about a ground-based Very Large Telescope picture of the cluster, seen here. The picture looks odd because Terzan 5 lies in a very crowded region of the Milky Way, lousy with dust. That interstellar junk tends to scatter away blue light, making objects look redder. The dust blankets across Terzan 5, but is thicker in one half than the other, making that side redder than the other.

Terzan 5 itself is also unusually dense, with stars packed in it more tightly than is usual for a globular cluster. Not only that, but studies have shown the stars in the cluster appear to fall into two different age groups; one significantly older than the other. That’s weird. In most clusters, the stars are all the same age, indicating the cluster formed all at once. Terzan 5 isn’t like that, so maybe it has a different birth story.

Astronomers think that the cluster may actually be the remains of a dwarf galaxy, one much smaller than ours, that got eaten by the Milky Way. Billions of years ago the two collided, and the gravity of our bigger galaxy stripped away many of the stars in Terzan 5. What was left over was this roughly spherically-shaped ball. The stars are different ages because some galaxies tend to form stars in bursts, making lots of stars, then not many, then lots of stars again as time goes on. That fits with what we see here.

So Terzan 5 is basically the undigested bits left over after a galactic cannibalism event.

The Hubble picture itself is pretty nifty, too. This is a little complicated, so bear with me. The image is false color: it’s a combination of two observations, one using a yellow filter (colored blue in the final shot here) and the other in the near infrared (colored red). The astronomers also simulated a third exposure by combining and processing the two observations to mimic what an observation through a green(ish) filter would have produced. By combining all three images, they get the results above. I don’t think creating that third quasi-green image produces much science, but it does make a pleasing picture.

It’s different than the VLT image; the striking difference in color across the VLT picture isn’t as obvious as in the Hubble picture. But if you look carefully you can see the streak of red stars going through the Hubble shot. The filters used and the way they were combined change the way we see the resulting image. And it’s more than just a pretty picture: in this case it helps understand how the stars are arranged in the cluster, and that provides clues to what happened to it in the past.

It’s not completely clear that Terzan 5 was once a galactic snack, it still may just be a very odd globular cluster. But by observing it using multiple telescopes in multiple ways we learn more about it, and hopefully will be able to unravel what happened all those eons ago to make this strange and lovely object.

Image Credits: NASA/ESA/Hubble; ESO/F. Ferraro
Gamma-ray emission from Terzan 5
Max Planck Gesellschaft | 2011 June 23
The discovery of a source in the direction of the globular cluster puzzles astrophysicists
The H.E.S.S. telescope system in Namibia discovered a new source of very-high-energy gamma-rays from the direction of the globular cluster Terzan 5. Being very likely located in the outer parts of Terzan 5 this source is the first example for of gamma-ray emission from a globular cluster. The off-centre position of the source and the specific origin of the gamma-rays pose a puzzle for scientists.

The globular cluster Terzan 5 situated in the Sagittarius constellation is a remarkable object in several aspects. Obscured behind galactic dust clouds the faint cluster was discovered in 1968 by Agop Terzan on photographic plates of the Haute-Provence Observatory in France. About 150 known globular clusters, concentrated spherical collection of very old stars, orbit the centre of our galaxy in form of a spherical swarm as part of the galactic halo.

Terzan 5 is located in the inner parts of our galaxy closely above the galactic plain in about 20,000 light-years distance to the earth. It has the highest density of stars of all globular clusters and contains the largest number of millisecond pulsars. The latter are rapidly rotating neutron stars which are thought to be part of close binary systems.

Terzan 5 gained particular attention in 2009 when it turned out that is has two star populations of different age (12 and 6 billion years, respectively). Due to these unique properties Terzan 5 is assumed to be the remnant of a dwarf galaxy which has been captured by our galaxy.

Researchers of the Max Planck Institute for Nuclear Physics in Heidelberg and 33 other institutions within the H.E.S.S. collaboration report the discovery of a new source (HESS J1747 – 248) of very-high-energy gamma-rays from the direction of Terzan 5. The location in the close vicinity to the cluster suggests that the source is a so far unknown part of Terzan 5. The probability of a chance coincidence with an unrelated gamma emission (derived from the abundance of known sources) is less than 1/10,000.

The photon energy of very-high-energy gamma-rays exceeds that of visible light by a factor of several trillions. The gamma-rays are detected by the H.E.S.S. (High Energy Stereoscopic System) Cherenkov telescope system in Namibia. It consists of four large telescopes equipped with ultrafast cameras which image extremely faint light (Cherenkov radiation) of atmospheric particle showers created by gamma photons absorbed about 10 km above the ground. Coincident observation from the up to four viewpoints allows to reconstruct the original direction of the gamma-ray source in the sky. Terzan 5 is the first case of a globular cluster being identified as a gamma-ray emitting object.

Like many discoveries, the new source raises a bunch of questions which are not finally settled up to now. One striking feature is the elongated form of the source and its significant offset from the cluster’s centre. There exist several explanations for the origin of the gamma-rays which have been discussed within studies of other known sources. Based on theoretical models it is assumed that first charged particles (electrons, protons) gain the according energy in a cosmic accelerator. The particle’s energy is then subsequently transformed into gamma photons in collision processes.

While millisecond pulsars may act as gamma-ray sources themselves, electron acceleration may be driven as well by pulsar winds or colliding shock fronts therein – plausible processes considering the high stellar density in a globular cluster. Indeed, diffuse X-ray emission from Terzan 5 has already been observed. However, this does not explain the offset of the gamma source from the centre of the cluster where one expects both the highest density of pulsars and the highest rate of electron interaction with stellar light.

Protons are known to be accelerated in supernova remnants and these spectacular explosions induced by stellar collisions are expected to occur in globular clusters as well. But again, there is the question why the source is found off-centre. The source object may have been ejected into the outer zone by a close stellar encounter. But it remains puzzling why HESS J1747 – 248 is a “dark source” which is not detectable so far in other regions of the electromagnetic spectrum. “In summary, the nature of the source is uncertain since no counterpart or model fully explains the observed morphology” says Wilfried Domainko from the Max Planck Institute of Nuclear Physics.

Future studies will concentrate on the region of less energetic gamma-rays which is still unexplored so far both by satellite-based measurements and observations by telescope systems like H.E.S.S. Currently, the construction of a fifth large telescope (H.E.S.S. II) is under way. By means of a fivefold larger mirror area of about 600 square metres it will be sensitive enough to detect the even more faint particle showers produced by less energetic photons.
Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5 - H.E.S.S. Collaboration
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NOVA: Neutron Star Blows Away Models for Thermonuclear Explo

Post by bystander » Wed Sep 14, 2011 9:48 pm

Neutron Star Blows Away Models for Thermonuclear Explosions
University of Amsterdam | via PhysOrg | 2011 Sept 14
Amsterdam astronomers have discovered a neutron star that confounds existing models for thermonuclear explosions in such extreme objects. In the case of the accreting pulsar IGR J17480-2446, it seems to be a strong magnetic field that causes some parts of the star to burn more brightly than the rest. The results of the study, by Yuri Cavecchi et al. (2011), are to be published in the journal Astrophysical Journal Letters.

The neutron star concerned is part of the X-ray binary IGR J17480-2446 (hereafter J17480). X-ray binaries consist of a neutron star and a companion star in orbit around each other. Neutron stars, which are about 1.5 times as massive as the Sun, with a diameter of about 25 km, have a strong gravitational field that can pull gas from the companion star. This gas can build up on the neutron star surface and explode in a fast, high-energy thermonuclear reaction. Normally, the entire surface of the star explodes uniformly. However, in about 10 percent of cases, some parts of the star become much brighter than the rest. Why this occurs is not understood.

In recent years a number of theoretical models have been developed to explain this phenomenon. According to one model, the rapid rotation of the neutron star prevents the burning material from spreading, just as the rotation of the Earth contributes to the formation of hurricanes via the Coriolis force. Another idea is that the explosion generates global-scale waves in the surface ‘ocean’ layers of the star. The ocean on one side of the star cools and dims as it rises up, while the other stays warmer and brighter.

The new study of J17480 excludes both of these models. Like other stars, J17480 develops unusually bright surface patches during thermonuclear explosions. However the star rotates much more slowly than other neutron stars that exhibit this behavior -- only 10 times per second (the next slowest rotates 245 times per second). At this speed, the Coriolis force is not strong enough to affect the flame front, preventing the formation of thermonuclear hurricanes. The development of large-scale ocean waves can also be ruled out.

Instead, the astronomers think that the magnetic field of the star might explain the uneven burning. The exploding gas expands, moving upwards and outwards. This churns up the magnetic field, which acts like an elastic band to prevent the burning bubble from spreading any further. “More theoretical work is needed to confirm this, but in the case of J17480 it is a very plausible explanation for our observations”, says lead author Yuri Cavecchi (University of Amsterdam, the Netherlands).

Co-author Anna Watts (University of Amsterdam) stressed that their new model may not necessarily explain non-uniform burning for all stars. “The new mechanism may only work in stars like this one, with magnetic fields that are strong enough to stop the flame front from spreading. For other stars with this odd burning behavior, the old models might still apply.”

Implications of burst oscillations from the slowly rotating accreting pulsar IGR 17480-2446 in the globular cluster Terzan 5 - Y. Cavecchi et al
  • arXiv.org > astro-ph > arXiv:1102.1548 > 08 Feb 2011 (v1), 22 Aug 2011 (v2)

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