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| Paper: |
The Stellar Content of the Galactic Center |
| Volume: |
186, The Central Parsecs of the Galaxy |
| Page: |
291 |
| Authors: |
Blum, R. D.; RamÃrez, S. V.; Sellgren, K. |
| Abstract: |
We briefly review the current stellar census of the bright end of the K-band luminosity function in the central few parsecs of the Milky Way. New H and K-band spectra are presented for a sample of cool stars. The broad H2O absorption feature near 1.9 microns can be used in combination with the 2.3 microns CO feature to distinguish between AGB and supergiant stars. |
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