A method for deriving accurate gas-phase abundances for the multiphase interstellar Galactic halo

Astrophysical Journal

Volumn 637, Issue 1 I, 2006, Pages 333-341

  Christopher Howk, J ^a,b   Sembach, Kenneth R ^c   Savage, Blair D ^d  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF NOTRE DAME   (United States)

^c AURA for the European Space Agency   (United States)

^d UNIVERSITY OF WISCONSIN MADISON   (United States)

Author keywords

ISM: atoms; ISM: structure; Ultraviolet: ISM

Indexed keywords

EID: 33644537664     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/497352     Document Type: Article

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