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ON THE RADIO PROPERTIES OF V645 CYGNI

SUN KWOK
Publications of the Astronomical Society of the Pacific
Vol. 93, No. 553 (June 1981), pp. 361-363
Stable URL: http://www.jstor.org/stable/40677779
Page Count: 3
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Since scans are not currently available to screen readers, please contact JSTOR User Support for access. We'll provide a PDF copy for your screen reader.
ON THE RADIO PROPERTIES OF V645 CYGNI
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Abstract

Upper limits of 0.5 mjy at 5 GHz and 4 mJy at 15 GHz have been obtained for the continuum flux densities of V645 Cyg. These low upper limits imply that any associated H II region must be extremely dense and compact, with angular size < 0.''06 and density > 3 × 10⁶cm. Alternatively, there may be a stellar wind associated with the star with a mass loss rate < 10⁵ 𝕸 ⊙ yr¹.

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