Issue |
A&A
Volume 376, Number 1, September II 2001
|
|
---|---|---|
Page(s) | 124 - 135 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20010931 | |
Published online | 15 September 2001 |
Adaptive optics
-band observations of the Galactic Center region
1
Observatoire de Paris, DESPA, 5 place Jules Janssen, 92190 Meudon, France
2
ONERA, 29 avenue de la Division Leclerc, BP 72, 92322 Chatillon Cedex, France
3
Gemini Observatory, 670 N. A'ohoku Place, Hilo, Hawaii, 96720, USA
Corresponding author: Y. Clénet, yann.clenet@obspm.fr
Received:
5
February
2001
Accepted:
20
June
2001
L-band adaptive optics observations of the Galactic Center region have been performed in June 1999 and May 2000 at La Silla with the 3.6 m telescope, using the ADONIS adaptive optics system. In June 1999, we used a dedicated infrared wave-front sensor, RASOIR. This paper reports on the photometry and astrometry of more than 40 stars. Thanks to additional adaptive optics K-band observations made at CFHT, colour-magnitude diagrams have been constructed to identify individual sources with various types of stars known in this region (AGB, LPV, WC9, WN9/WN10, Ofpe/WN9, YSO). The so-called "cool slash" stars (Ofpe/WN9) appear to be numerous in the field and an estimation of the extinction coefficient towards the Galactic Center from the colours of these intrinsically weakly absorbed stars leads to AK=2.7, which is among the lowest published values.
Key words: instrumentation: adaptive optics / Galaxy: center / infrared: stars / ISM: dust, extinction / stars: population II
© ESO, 2001
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