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• W1963837241 abstract "We 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." @default.
• W1963837241 created "2016-06-24" @default.
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• W1963837241 date "2005-03-04" @default.
• W1963837241 modified "2023-10-18" @default.
• W1963837241 title "Interferometric Observations of V838 Monocerotis" @default.
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• W1963837241 doi "https://doi.org/10.1086/429619" @default.
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