On the fate of Galactic Centre molecular clouds
Open Access
- 1 January 1991
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 248 (1) , 14P-17P
- https://doi.org/10.1093/mnras/248.1.14p
Abstract
One third of the CO-emitting gas within 500 pc of the Galactic Center is in a few massive clouds. If these clouds have masses of the expected order $$(3\times{10}^{6}{M}_{\odot})$$, even the outermost is doomed to spiral into the center within a Gyr. The subsequent evolution is unclear, but it will almost certainty be violent. This suggests that the Galactic center is subjected to starbursts.
This publication has 0 references indexed in Scilit: