Late-type star spectra (Montes+ 1997)

Details Late-type star spectra (Montes+ 1997) Late-type star spectra (Montes+ 1997)

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..41230473m&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/123/473. Originally published in: 1997A&AS..123..473M

Physics

Spectroscopy, Stars: Late-Type

Scientific paper

In this work we present spectroscopic observations centered in the spectral lines most widely used as optical indicators of chromospheric activity (Hα, Hβ, Ca II H & K, and He I D{3}) in a sample of F, G, K and M chromospherically inactive stars. The spectra have been obtained with the aim of providing a library of high and mid-resolution spectra 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 (1 data file).

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