Abstract
We have observed the metal-rich globular cluster NGC 6356 in the CO J = 2 → 1 transition. The data revealed no apparent emission corresponding to the radial velocity of the cluster and we present an upper limit to the mass of gas in the cluster core.
Original language | English |
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Pages (from-to) | 385-388 |
Number of pages | 4 |
Journal | Astrophysics and Space Science |
Volume | 251 |
Issue number | 1-2 |
DOIs | |
Publication status | Published - 1997 |