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A&A 437, L1-L5 (2005)
DOI: 10.1051/0004-6361:200500126
Letter
Current day mass loss rate for Luminous Blue Variable IRAS 18576+0341
G. Umana1, 2, C. S. Buemi2, C. Trigilio2 and P. Leto21 INAF - Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania Italy
2 INAF - Istituto di Radioastronomia Sezione di Noto, CP 141, 96017 Noto (SR), Italy
e-mail: g.umana@ira.inaf.it
(Received 23 February 2005 / Accepted 13 May 2005 )
Abstract
In this letter we report on the first set of multi-frequency and high angular resolution radio observations of
IRAS 18576+0341
.
The radio observations have revealed an extended, asymmetric and quite structured radio nebula
and allowed us to locate the central core of this highly obscured new galactic Luminous Blue Variable. From the analysis of radio properties of
IRAS 18576+0341
estimates of important physical parameters of the central star have been determined. In particular, an effective temperature of
, corresponding to a B0-B0.5 supergiant, has been derived.
The most notable result is the determination of the current
day mass-loss (
), which is of particular
importance since mass-loss rate determination from radio observations appears to be a more reliable
method compared to the others based on different diagnostics.
Key words: circumstellar matter -- stars: winds, outflows -- stars: mass-loss -- radio continuum: stars -- stars: individual: IRAS 18576+0341, AFGL 2298
SIMBAD Objects in preparation
© ESO 2005
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