Possible Dishevelled Structure of Wolf-Rayet Atmospheres

Details Possible Dishevelled Structure of Wolf-Rayet Atmospheres Possible Dishevelled Structure of Wolf-Rayet Atmospheres

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986atsir1460....1a&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1460/OCT, 1986

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Ionization state calculations of WR atmospheres have been carried out which demonstrate that the simultaneous co-existence of He+ and He++ (and other) zones of ionization is possible only in a very narrow range of Teff: ΔTeff ≈ 2000K. This result is in contradiction with observations. The contradiction can be removed assuming a dishevelled structure of WR atmospheres consisting of dense "clouds" and low-density "intercloud" matter.

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