FU orionis resolved by infrared long-baseline interferometry at a 2 AU scale

Astrophysical Journal

Volumn 507, Issue 2 PART II, 1998, Pages

  Malbet, F ^a   Berger, J P ^a   Colavita, M M ^b   Koresko, C D ^c   Beichman, C ^b,d   Boden, A F ^b   Kulkarni, S R ^c   Lane, B F ^c   Mobley, D W ^b   Pan, X P ^c   Shao, M ^b   Van Belle, G T ^b   Wallace, J K ^b  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Accretion, accretion disks; Circumstellar matter; Infrared: stars; Instrumentation: interferometers; Stars: individual (FU Orionis); Stars: pre main sequence

Indexed keywords

EID: 0039400217     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/311688     Document Type: Article

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