ESO: Best View of Cloud Passing Galactic Center Black Hole

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bystander
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ESO: Best View of Cloud Passing Galactic Center Black Hole

Post by bystander » Thu Mar 26, 2015 10:29 pm

Best View Yet of Dusty Cloud Passing Galactic Center Black Hole
ESO Science Release | VLT | 2015 Mar 26

VLT observations confirm that G2 survived close approach and is a compact object
[imghover=http://www.eso.org/public/archives/imag ... o1512a.jpg]http://www.eso.org/public/archives/imag ... o1512b.jpg[/imghover][c]The dusty cloud G2 passes the supermassive black hole
at the centre of the Milky Way (Credit: ESO/A. Eckart)
[/c]

The best observations so far of the dusty gas cloud G2 confirm that it made its closest approach to the supermassive black hole at the centre of the Milky Way in May 2014 and has survived the experience. The new result from ESO’s Very Large Telescope shows that the object appears not to have been significantly stretched and that it is very compact. It is most likely to be a young star with a massive core that is still accreting material. The black hole itself has not yet shown any increase in activity.

A supermassive black hole with a mass four million times that of the Sun lies at the heart of the Milky Way galaxy. It is orbited by a small group of bright stars and, in addition, an enigmatic dusty cloud, known as G2, has been tracked on its fall towards the black hole over the last few years. Closest approach, known as peribothron, was predicted to be in May 2014.

The great tidal forces in this region of very strong gravity were expected to tear the cloud apart and disperse it along its orbit. Some of this material would feed the black hole and lead to sudden flaring and other evidence of the monster enjoying a rare meal. To study these unique events, the region at the galactic centre has been very carefully observed over the last few years by many teams using large telescopes around the world. ...

Monitoring the Dusty S-Cluster Object (DSO/G2) on its Orbit towards the Galactic Center Black Hole - M. Valencia-S. et al
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