The distance to the supernova remnant CTB 87 and the radial velocity of the perseus arm toward l = 75°, derived from H i and CO observations

Astrophysical Journal

Volumn 588, Issue 2 I, 2003, Pages 852-861

  Kothes, Roland ^a,b   Reich, Wolfgang ^c   Foster, Tyler ^a,d   Byun, Do Young ^e  

^a NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^b UNIVERSITY OF CALGARY   (Canada)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^d UNIVERSITY OF ALBERTA   (Canada)

^e Seoul National University   (South Korea)

Author keywords

Galaxy: kinematics and dynamics; ISM: clouds; ISM: individual (CTB 87); ISM: kinematics and dynamics; Supernova remnants

Indexed keywords

EID: 0043263887     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/374219     Document Type: Article

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