From what Radius do the Winds of Magellanic Cloud Supergiants Produce Feii Emission Lines

Details From what Radius do the Winds of Magellanic Cloud Supergiants Produce Feii Emission Lines From what Radius do the Winds of Magellanic Cloud Supergiants Produce Feii Emission Lines

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..235f&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

1

Scientific paper

Maximum values for the inner radii at which Fe II emission line
formation can take place in the winds of three Magellanic Cloud
supergiants have been determined. They lie between
3×1013cm and 3×1014 cm for R50, R82,
and R126.

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