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Sgr A* envelope explosion and the young stars in the centre of the Milky Way
journal contribution
posted on 2018-08-10, 14:50 authored by Sergei Nayakshin, Kastytis ZubovasSgr A* is the supermassive black hole residing in the centre of the Milky Way. There is plenty of observational evidence that a massive gas cloud fell into the central parsec of the Milky Way ∼6 Myr ago, triggering formation of a disc of young stars and activating Sgr A*. In addition to the disc, there is an unexplained population of young stars on randomly oriented orbits. Here we hypothesize that these young stars were formed by fragmentation of a massive quasi-spherical gas shell driven out from Sgr A* potential well by an energetic outflow. To account for the properties of the observed stars, the shell must be more massive than 105 solar masses, be launched from inside ∼0.01 pc, and the feedback outflow has to be highly super-Eddington albeit for a brief period of time, producing kinetic energy of at least 1055 erg. The young stars in the central parsec of the Galaxy may be a unique example of stars formed from atomic rather than molecular hydrogen, and forged by extreme pressure of black hole outflows.
Funding
KZ is funded by the Research Council Lithuania through the grant no. MIP-17-78. SN acknowledges support by STFC grant ST/K001000/1.
History
Citation
Monthly Notices of the Royal Astronomical Society: Letters, 2018, 478(1) pp. L127–L131.Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and AstronomyVersion
- VoR (Version of Record)
Published in
Monthly Notices of the Royal Astronomical Society: LettersPublisher
Oxford University Press (OUP), Royal Astronomical Societyeissn
1745-3933Acceptance date
2018-04-23Copyright date
2018Available date
2018-08-10Publisher DOI
Publisher version
https://academic.oup.com/mnrasl/article/478/1/L127/4996354Language
enAdministrator link
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