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Volumn 474, Issue 2, 2007, Pages 591-597

Identification of Ne VIII lines in H-deficient (pre-) white dwarfs: A new tool to constrain the temperature of the hottest stars

Author keywords

Stars: abundances; Stars: AGB and post AGB; Stars: atmospheres; Stars: evolution; White dwarfs

Indexed keywords

ABSORPTION SPECTRA; ASTROPHYSICS; CONSTRAINT THEORY; LIGHT EMISSION; NEON; WIND;

EID: 35549000177     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078152     Document Type: Article
Times cited : (40)

References (33)
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    • Rauch, T.1    Werner, K.2
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    • Werner, K.1    Heber, U.2
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    • Werner, K., Heber, U., & Hunger, K. 1991, A&A, 244, 437 Werner, K., Hamann, W-R., Heber, U., et al. 1992, A&A, 259, L69
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.