A new phase of activity of the Herbig Be star HD 200775 in 2001: Evidence for binarity

Astronomy and Astrophysics

Volumn 417, Issue 2, 2004, Pages 715-723

  Pogodin, M A ^a,b   Miroshnichenko, A S ^a,c   Tarasov, A E ^d,e   Mitskevich, M P ^d,e   Chountonov, G A ^f   Klochkova, V G ^f   Yushkin, M V ^f   Manset, N ^g   Bjorkman, K S ^c   Morrison, N D ^c   Wisniewski, J P ^c  

^a RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^b Isaac Newton Institute of Chile   (Russian Federation)

^c UNIVERSITY OF TOLEDO   (United States)

^d CRIMEAN ASTROPHYSICAL OBSERVATORY   (Ukraine)

^e Isaak Newton Institute of Chile   (Ukraine)

^f RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^g CANADA FRANCE HAWAII TELESCOPE   (United States)

Author keywords

Stars: binaries: spectroscopic; Stars: circumstellar matter; Stars: individual: HD 200775; Stars: pre main sequence; Techniques: spectroscopic

Indexed keywords

INFORMATION ANALYSIS; INTERFEROMETRY; LIGHT EMISSION; MODAL ANALYSIS; OPTICAL TELESCOPES; PARAMETER ESTIMATION; SIGNAL TO NOISE RATIO; SPECTROSCOPIC ANALYSIS;

STARS: BINARIES: SPECTROSCOPIC; STARS: CIRCUMSTELLAR MATTER; STARS: INDIVIDUAL: HD 200775; STARS: PRE-MAIN SEQUENCE; TECHNIQUES: SPECTROSCOPIC;

ASTRONOMY;

EID: 11144355205     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031783     Document Type: Article

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