Modelling chromospheric line profiles as diagnostics of velocity fields inω Centauri red giant stars-Reference-Cited by-同舟云学术

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Modelling chromospheric line profiles as diagnostics of velocity fields inω Centauri red giant stars

Published:2010-12-10 Issue: Volume:526 Page:A4
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Vieytes M.,Mauas P.,Cacciari C.,Origlia L.,Pancino E.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201015455/pdf

Reference79 articles.

1. Helium Line Formation and Abundance during a C‐Class Flare

2. Avrett, E. H., & Loeser, R. 1984, in Methods in Radiative Transfer, ed. W. Kalkofen (Cambridge Univ. Press), 341

3. ASPITZERSEARCH FOR COLD DUST WITHIN GLOBULAR CLUSTERS

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