Library of high-resolution UES echelle spectra of F, G, K and M field dwarf stars

被引：43

作者：

Montes, D ^{[1
]}

Martin, EL

机构：

[1] Univ Complutense Madrid, Fac Fis, Dept Astrofis, E-28040 Madrid, Spain

[2] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[3] Inst Astrofis Canarias, E-38200 La Laguna, Spain

[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1998年 / 128卷 / 03期

关键词：

atlases; stars; activity; chromospheres; late-type; fundamental parameters; general;

D O I：

10.1051/aas:1998159

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a library of Utrecht echelle spectrograph (UES) observations of a sample of F, G, K and M field dwarf stars covering the spectral range from 4800 Angstrom to 10600 Angstrom with a resolution of 55000. These spectra include some of the spectral lines most widely used as optical and near-infrared indicators of chromospheric activity such as H beta, Mg I b triplet, Na I D-1, D-2, He I D-3, H alpha, and Ca II IRT lines, as well as a large number of photospheric lines which can also be affected by chromospheric activity. The spectra have been compiled with the aim of providing a set of standards observed at high-resolution to be used in the application of the spectral subtraction technique to obtain the active-chromosphere contribution to these lines in chromospherically active single and binary stars. This library can also be used for spectral classification purposes. A digital version with all the spectra is available via ftp and the World Wide Web (WWW) in both ASCII and FITS formats.

引用

页码：485 / 495

页数：11

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