Issue |
A&A
Volume 366, Number 3, February II 2001
|
|
---|---|---|
Page(s) | 1003 - 1007 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20000331 | |
Published online | 15 February 2001 |
High resolution spectroscopy over 8500-8750 Åfor GAIA *,**,***
III. A library of synthetic spectra for 7750≤ 50 000 K
1
CNR-GNA-Osservatorio Astronomico di Trieste Via Tiepolo 11, 34131 Trieste, Italy
2
Osservatorio Astronomico di Padova, Sede di Asiago, 36012 Asiago (VI), Italy
3
Centro Interpardimentale Studi ed Attività Spaziali (CISAS "G. Colombo"), Università di Padova, Italy
Corresponding author: U. Munari, munari@pd.astro.it
Received:
8
September
2000
Accepted:
23
November
2000
In this paper we complete the library of synthetic spectra for the range 7650-8750 Å, which includes the 8500-8750 Åinterval currently base-lined for the spectroscopic observations by GAIA, candidate ESA Cornerstone 5 mission. As for Paper II, the spectra are based on Kurucz's codes and line data. The explored metallicity, gravity and temperature ranges are , and K, respectively. The 698 new spectra are computed at the same resolving power of the observed spectra given in Paper I (131 standard stars mapping the MKK spectral classification system) and the 254 synthetic spectra of Paper II (characterized by K).
Key words: atlases / surveys / stars: fundamental parameters
© ESO, 2001
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