Explaining UX orionis star variability with self-shadowed disks

Astrophysical Journal

Volumn 594, Issue 1 II, 2003, Pages

  Dullemond, C P ^a   Van den Ancker, M E ^b   Acke, B ^c   Van Boekel, R ^d  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c KU LEUVEN   (Belgium)

^d Sterrenkundig Inst Anton Pannekoek   (Netherlands)

Author keywords

Circumstellar matter; Planetary systems: protoplanetary disks; Stars: pre main sequence; Stars: variables: other

Indexed keywords

EID: 0141792532     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/378400     Document Type: Review

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