Tracing the young massive high-eccentricity binary system θ1 Orionis C through periastron passage

Astronomy and Astrophysics

Volumn 497, Issue 1, 2009, Pages 195-207

  Kraus, S ^a   Weigelt, G ^a   Balega, Y Y ^b   Docobo, J A ^c   Hofmann, K H ^a   Preibisch, T ^d   Schertl, D ^a   Tamazian, V S ^c   Driebe, T ^a   Ohnaka, K ^a   Petrov, R ^e   Scholler M ^f   Smith, M ^g  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^c UNIVERSITY OF SANTIAGO DE COMPOSTELA   (Spain)

^d UNIVERSITY OF MUNICH   (Germany)

^e UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^g UNIVERSITY OF KENT   (United Kingdom)

Author keywords

Binaries: close; Stars: formation; Stars: fundamental parameters; Stars: imaging; Stars: individual: 1Orionis C; Techniques: interferometric

Indexed keywords

BINARIES: CLOSE; STARS: FORMATION; STARS: FUNDAMENTAL PARAMETERS; STARS: IMAGING; TECHNIQUES: INTERFEROMETRIC;

AMBER; GEOMETRICAL OPTICS; INTERFEROMETERS; OPTICAL TELESCOPES; ORBITS; SPECKLE; STARS; SYSTEMS (METALLURGICAL); TELESCOPES; VELOCITY MEASUREMENT;

INTERFEROMETRY;

EID: 63849201631     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810368     Document Type: Article

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