Image of fomalhaut dust ring at 350 microns: The relative column density map shows pericenter-apocenter asymmetry

Astrophysical Journal

Volumn 620, Issue 1 II, 2005, Pages

  Marsh, K A ^a   Velusamy, T ^a   Dowell, C D ^a   Grogan, K ^a   Beichman, C A ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Circumstellar matter; Planetary systems; Stars: individual (fomalhaut)

Indexed keywords

EID: 15944389535     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/428401     Document Type: Article

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