Library of high and mid-resolution spectra in the
CaII H & K, H
,
H
,
and NaI D1,
D2,
and HeI D3 lines regions
of F, G, K and M field stars
|
D. Montes1, E.L. Martín2, M.J. Fernández-Figueroa1, M. Cornide1, E. De Castro1,
1
Departamento de Astrofísica, UCM
2
Instituto de Astrofísica de Canarias
(accepted September 1996)
1997, Astronomy & Astrophysics Supplement Series, (Jun II), 123, 473
PS_file (gzip)
-- 
Available at CDS (J/A+AS/123/473)
Full Version in HTML
In this work we present spectroscopic observations
centered in the spectral lines most widely used as
optical indicators of chromospheric activity
(H,
H, CaII H & K, and
and HeI D3)
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.
CaII H & K line region
H line region
- high-resolution spectra (spectral resolution, 0.3 - 0.5 Ĺ)
- mid-resolution spectra (spectral resolution, 0.8 - 1.0 Ĺ)
H line region
NaI D1,
D2,
and HeI D3 line region
H +
NaI D1,
D2
line region
Tables with the summary of the observations
(Paper II),
Library of high-resolution UES echelle spectra
of F, G, K and M field dwarf stars,
(Montes & Martín 1998, A&AS 128, 485)
(Paper III),
Library of medium-resolution Fiber Optic Echelle spectra
of F, G, K and M field dwarfs to giants stars
(Montes, Ramsey, & Welty, 1999, ApJS 123, 283)
Late-M and L Field Dwarfs Spectra
from "Spectroscopic Classification of Late-M and L Field Dwarfs",
(Martín E.L. et al., 1999, AJ 118, 2466)
Other Libraries of stellar spectra
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