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

Publisher： Edp Sciences

E-ISSN： 1432-0746|434|2|707-712

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.434, Iss.2, 2005-05, pp. : 707-712

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