Publications
of the
MPIfR
Optical & Infrared
Interferometry Group
K.-H. Hofmann, N.R. Ikhsanov, G. Weigelt, A.S.
Miroshnichenko
Bispectrum speckle interferometry of the B(e) star MWC 349A
Astronomische Gesellschaft Abstract Series (AGM 19,
P42)
Der kosmische Materiekreislauf
Annual Scientific Meeting of the Astronomische Gesellschaft, Sep 23-28,
2002, Berlin, Germany
Abstract
We present the results of bispectrum speckle interferometry of the B[e] star MWC 349A obtained with the SAO 6m telescope. Our diffraction-limited J-, H-, and K-band images (resolutions 43-74 mas) suggest the star is surrounded by a circumstellar disk seen almost edge-on. The observed visibility shape is consistent with a two-component elliptical disk model, probably corresponding to the gaseous and dusty components of the disk. We show that the classification of the object as a pre-main-sequence star or a young planetary nebula is problematic. An analysis of the uncertainties in the basic parameter determination lead us to the conclusion that MWC 349A is probably either a B[e] supergiant or a binary system, in which the B[e]-companion dominates the observed properties.
| slilley@mpifr-bonn.mpg.de |
Back to Group
Home Page |