Issue |
A&A
Volume 406, Number 3, August II 2003
|
|
---|---|---|
Page(s) | 995 - 999 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20030647 | |
Published online | 17 November 2003 |
High resolution spectroscopy over
8500-8750 Å for GAIA*
IV. Extending the cool MK stars sample
1
Padova Astronomical Observatory - INAF, Asiago Station, Via Osservatorio 8, 36012 Asiago (VI), Italy e-mail: marrese@pd.astro.it, boschi@pd.astro.it
2
Department of Astronomy, University of Padova, Vicolo Osservatorio 8, 35122 Padova, Italy
Corresponding author: U. Munari, munari@pd.astro.it
Received:
12
December
2002
Accepted:
24
April
2003
A library of high resolution spectra of MK standard and reference stars, observed in support to the GAIA mission, is presented. The aim of this paper is to integrate the MK mapping of Paper I of this series as well as to consider stars over a wider range of metallicities. Radial velocities are measured for all the target stars.
Key words: atlases / standards / stars: fundamental parameters
The spectra are available in electronic form (ASCII format) at CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/406/995 and from the web page http://ulisse.pd.astro.it/MoreMK/, where further bibliographical information for the target stars is given.
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.