The properties of molecular hydrogen toward the orion belt stars from observations by the interstellar medium absorption profile spectrograph

Astrophysical Journal

Volumn 538, Issue 1 PART 1, 2000, Pages 275-288

  Jenkins, Edward B ^a   Woźniak, Przemyslaw R ^a   Sofia, Ulysses J ^b,c   Sonneborn, George ^d   Tripp, Todd M ^a  

^a PRINCETON UNIVERSITY OBSERVATORY   (United States)

^b VILLANOVA UNIVERSITY   (United States)

^c WHITMAN COLLEGE   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

ISM: molecules; Stars: individual ( Orionis A, Orionis, Orionis A); Ultraviolet: ISM

Indexed keywords

EID: 0034691380     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309130     Document Type: Article

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