Resolving the asymmetric inner wind region of the yellow hypergiant IRC +10420 with VLTI/AMBER in low and high spectral resolution mode

Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages 301-316

  Driebe, T ^a   Groh, J H ^a   Hofmann, K H ^a   Ohnaka, K ^a   Kraus, S ^a   Millour, F ^a   Murakawa, K ^a   Schertl, D ^a   Weigelt, G ^a   Petrov, R ^b   Wittkowski, M ^c   Hummel, C A ^c   Le Bouquin, J B ^d   Merand, A ^d   Scholler M ^c   Massi, F ^e   Stee, P ^b   Tatulli, E ^f  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f UNIV GRENOBLE ALPES   (France)

Author keywords

Instrumentation: high angular resolution; Instrumentation: interferometers; Stars: circumstellar matter; Stars: individual: IRC +10 420; Stars: mass loss; Stars: supergiants

Indexed keywords

INSTRUMENTATION: INTERFEROMETERS; INSTRUMENTATION:HIGH ANGULAR RESOLUTION; STARS: CIRCUMSTELLAR MATTER - STARS; STARS: MASS-LOSS; STARS: SUPERGIANTS;

AMBER; DUST; ELECTROMAGNETIC WAVE EMISSION; FLUORINE CONTAINING POLYMERS; INSTRUMENTS; INTERFEROMETERS; INTERFEROMETRY; OPTICAL TELESCOPES; RADIATIVE TRANSFER; SPECTRAL RESOLUTION; STARS; TRANSFER MOLDING; VISIBILITY;

RELAY CONTROL SYSTEMS;

EID: 70449674484     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911723     Document Type: Article

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