Line identification in soft X-ray spectra of stellar coronae by comparison with the hottest white dwarf's photosphere: Procyon, α Cen A+B, and H 1504+65-Reference-Cited by-同舟云学术

Line identification in soft X-ray spectra of stellar coronae by comparison with the hottest white dwarf's photosphere: Procyon, α Cen A+B, and H 1504+65

Published:2005-04-11 Issue:2 Volume:434 Page:707-712
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Werner K.,Drake J. J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20042057/pdf

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