B. F. Lane et al 2005 ApJ 622 L137 doi:10.1086/429619
B. F. Lane1, A. Retter2, R. R. Thompson3 and J. A. Eisner4
Show affiliationsWe have used long-baseline near-IR interferometry to resolve the peculiar eruptive variable star V838 Mon and to provide the first direct measurement of its angular size. Assuming a uniform disk model for the emission, we derive an apparent angular diameter at the time of observations (2004 November-December) of 1.83 ± 0.06 mas. For a nominal distance of 8 ± 2 kpc, this implies a linear radius of 1570 ± 400 R
. However, the data are somewhat better fitted by elliptical disk or binary component models, and we suggest that the emission may be strongly affected by ejecta from the outburst.
stars: individual (V838 Monocerotis); techniques: interferometric
Issue 2 (2005 April 1)
Received 2005 January 12, accepted for publication 2005 February 14
Published 2005 March 4
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