Variations of the high-level Balmer line spectrum of the helium-strong star σ Orionis E

Astronomy and Astrophysics

Volumn 475, Issue 3, 2007, Pages 1027-1037

  Smith, M A ^a,c   Bohlender, D A ^b  

^a CATHOLIC UNIVERSITY OF AMERICA   (United States)

^b NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^c STScI   (United States)

Author keywords

Stars: circumstellar matter; Stars: early type; Stars: individual: Orionis E; Stars: magnetic fields; Stars: winds, outflows; Ultraviolet: stars

Indexed keywords

BALMER EDGE; BALMER LINE SPECTRUM; HIGH-RESOLUTION SPECTRA; ORIONIS;

CONTINUUM MECHANICS; GASES; HELIUM; MAGNETOSPHERE; SPECTRUM ANALYSIS; THERMODYNAMICS;

STARS;

EID: 36549038641     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078196     Document Type: Article

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