Properties of the δ scorpii circumstellar disk from continuum modeling

Astrophysical Journal

Volumn 652, Issue 2 I, 2006, Pages 1617-1625

  Carciofi, A C ^a   Miroshnichenko, A S ^b,c   Kusakin, A V ^d,e   Bjorkman, J E ^c   Bjorkman, K S ^c   Marang, F ^f   Kuratov, K S ^e   Garcia Lario P ^g   Perea Calderon J V ^g   Fabregat, J ^h   Magalhaes A M ^a  

^a UNIVERSITY OF SÃO PAULO   (Brazil)

^b UNIVERSITY OF NORTH CAROLINA AT GREENSBORO   (United States)

^c UNIVERSITY OF TOLEDO   (United States)

^d MOSCOW STATE UNIVERSITY   (Russian Federation)

^e Fesenkov Astrophysical Institute   (Kazakhstan)

^f SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^g EUROPEAN SPACE AGENCY   (Spain)

^h UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Circumstellar matter; Methods: numerical; Stars: emission line, be; Stars: individual ( Scorpii); Techniques: photometric; Techniques: polarimetric

Indexed keywords

EID: 33845893915     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/507935     Document Type: Article

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