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Criteria for spectral classification of cool stars using high-resolution spectra

Published online by Cambridge University Press:  01 August 2006

David Montes
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected]
Raquel M. Martínez-Arnáiz
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected]
Jesus Maldonado
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected] Departamento de Física Teórica, C-XI, Facultad de Ciencias, Universidad Autónoma de Madrid, Cantoblanco, Spain
Juan Roa-Llamazares
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected]
Javier López-Santiago
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected] INAF – Osservatorio Astronomico di Palermo Giuseppe S. Vaiana, Piazza Parlamento 1, I-90134, Palermo, Italy email: [email protected]
Inés Crespo-Chacón
Affiliation:
Departamento de Astrofísica, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain email: [email protected]
Enrique Solano
Affiliation:
INTA – Laboratorio de Astrofísica Espacial y Física Fundamental, P.O. Box 50727, E-28080 Madrid, Spain email: [email protected]
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We have compiled a large number of optical spectra of cool stars taken with different high-resolution echelle spectrographs (R ≃ 40 000). Many of those are available as spectral libraries (Montes et al. 1997, 1998, 1999, <http://www.ucm.es/info/Astrof/invest/actividad/spectra.html)>.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007