VLTI + MIDI Study of the High Mass Protostellar Candidate NGC 3603 IRS 9A

Details VLTI + MIDI Study of the High Mass Protostellar Candidate NGC 3603 IRS 9A VLTI + MIDI Study of the High Mass Protostellar Candidate NGC 3603 IRS 9A

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010rmxac..38...71n&link_type=abstract

The Interferometric View on Hot Stars (Eds. Th. Rivinius & M. Curé) Revista Mexicana de Astronomía y Astrofísica (Serie de Confe

Astronomy and Astrophysics

Astrophysics

Stars: Early-Type, Stars: Formation, Stars: Pre-Main Sequence, Techniques: High Angular Resolution, Techniques: Interferometric

Scientific paper

The formation and early evolution of high mass stars is among the hottest topics in astrophysics. Interferometric studies of these young stars and their circumstellar environments (envelopes, disks and jets) at near and mid infrared wavelengths are still rare and in terms of data analysis/interpretation very challenging. We here report on observations of the high mass protostellar candidate NGC 3603 IRS 9A which we undertook with VLTI + MIDI in 2005, complemented by near and mid infrared imaging and spectroscopic data. We discuss our results obtained from dedicated modeling efforts, employing both DUSTY and MC3D radiative transfer codes for a selected number of source geometries and surface brightness distributions.

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