More Nitrogen Sequence Wr-Stars with OVI Doublet Lambda 3811 and Lambda 3834

Details More Nitrogen Sequence Wr-Stars with OVI Doublet Lambda 3811 and Lambda 3834 More Nitrogen Sequence Wr-Stars with OVI Doublet Lambda 3811 and Lambda 3834

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...238l...1n&link_type=abstract

Astronomy and Astrophysics, Vol. 238, NO. NOVI, P. L1, 1990

Astronomy and Astrophysics

Astrophysics

3

Stars: Wolf-Rayet, Stars: Individual, Lines: Identification, Lines: Profiles

Scientific paper

Using the spectra of 5 WR stars we show that in the case of WN stars the OVI doublet λλ 3811, 3834 Å known to appear in WC stars may be also an important feature. P Cygni absorption of OVI λ 3811 Å overlapped with the HeII+HI blend at λ 3796 Å probably explains the absence of the latter blend in the spectra of some WN stars.

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