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Radio Emission from HD167362 and Vy2–2

Nature Physical Science volume 245, pages 6–7 (1973)Cite this article

Abstract

MANY early-type emission-line stars exhibit a pronounced excess of infrared radiation. This may arise from thermal reradiation by circumstellar dust, although in some cases the infrared spectra indicate that free-free emission by circumstellar gas may be the predominant mechanism1–3. We have attempted to measure the radio emission from several such objects as a means of setting constraints on the latter hypothesis. Here we report the detection of radio emission from HD167362=MWC288 and from Vyssotsky 2–2=Minkowski 1–70.

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Authors and Affiliations

  1. CRESS and Department of Physics, York University, Toronto

    C. R. PURTON, P. A. FELDMAN & K. A. MARSH

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  1. C. R. PURTON
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  2. P. A. FELDMAN
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  3. K. A. MARSH
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PURTON, C., FELDMAN, P. & MARSH, K. Radio Emission from HD167362 and Vy2–2. Nature Physical Science 245, 6–7 (1973). https://doi.org/10.1038/physci245006a0

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