JHU: GISMO Reveals Cosmic 'Candy Cane'

Find out the latest thinking about our universe.
Post Reply
User avatar
bystander
Apathetic Retiree
Posts: 21576
Joined: Mon Aug 28, 2006 2:06 pm
Location: Oklahoma

JHU: GISMO Reveals Cosmic 'Candy Cane'

Post by bystander » Thu Dec 19, 2019 6:46 pm

New Space Image Reveals Cosmic 'Candy Cane'
Johns Hopkins University | 2019 Dec 18
Click to view full size image 1 or image 2
The central zone of our galaxy hosts the Milky Way’s largest, densest collection of giant
molecular clouds, raw material for making tens of millions of stars. This image combines
archival infrared (blue), radio (red) and new microwave observations (green) from the
Goddard-developed GISMO instrument. The composite image reveals emission from cold
dust, areas of vigorous star formation, and filaments formed at the edges of a bubble
blown by some powerful event at the galaxy’s center. Credit: NASA/GSFC

Deep in our Milky Way galaxy’s center, a candy cane emerges as the centerpiece of a new, colorful composite image from a NASA camera, just in time for the holidays.

The image—captured by a NASA-designed and built instrument called the Goddard-IRAM Superconducting 2-Millimeter Observer, or GISMO—shows the inner part of our galaxy, which hosts the largest, densest collection of giant molecular clouds in the Milky Way. These vast, cool clouds contain enough dense gas and dust to form tens of millions of stars like the Sun. The view spans a part of the sky about 1.5 degrees across, equivalent to roughly three times the apparent size of the Moon. ...

The studies detail how, after spending 8 hours looking at the sky and collecting data, GISMO detected the most prominent radio filament in the galactic center, making this the shortest wavelength where these curious structures have been observed. Scientists say the filaments delineate the edges of a large bubble produced by some energetic event at the galactic center. ...

The image is a composite of different color codes for emission mechanisms. Blue and cyan features reveal cold dust in molecular clouds where star formation is still in its infancy. Yellow features reveal the presence of ionized gas and show well-developed star factories; this light comes from electrons that are slowed but not captured by gas ions, a process also known as free-free emission. Red and orange regions show areas where synchrotron emission occurs, such as in the prominent Radio Arc and Sagittarius A, the bright source at the galaxy’s center that hosts its supermassive black hole. ...

GISMO Maps Inner Milky Way, Sees Cosmic ‘Candy Cane’
NASA | GSFC | 2019 Dec 18

New Image of Candy Cane-Shaped Feature in Center of Milky Way
University of California, Los Angeles | 2019 Dec 18

2 mm GISMO Observations of the Galactic Center. I. Dust Emission ~ Richard G. Arendt et al 2 mm GISMO Observations of the Galactic Center. II. A Nonthermal
Filament in the Radio Arc and Compact Sources
~ Johannes Staguhn et al
Know the quiet place within your heart and touch the rainbow of possibility; be
alive to the gentle breeze of communication, and please stop being such a jerk.
— Garrison Keillor

User avatar
neufer
Vacationer at Tralfamadore
Posts: 18805
Joined: Mon Jan 21, 2008 1:57 pm
Location: Alexandria, Virginia

Re: JHU: GISMO Reveals Cosmic 'Candy Cane'

Post by neufer » Thu Dec 19, 2019 7:34 pm

https://en.wikipedia.org/wiki/Gizmo_key wrote:

<<The gizmo key is a key commonly found on the B foot joint of certain models of flute. It closes the low B tone hole without closing the low C tone hole or the low C♯ tone hole, which is intended to facilitate the performance of the fourth octave C.

The gizmo key was introduced by Verne Q. Powell (Powell Flutes), in response to criticisms of the B foot joint by performers such as Jean-Pierre Rampal, who believed that the lengthened tube made it harder for them to produce the highest notes. It is now common on the instrument.>>
Art Neuendorffer

Post Reply