Near infrared spectra of galactic and Magellanic Wolf-Rayet stars

Details Near infrared spectra of galactic and Magellanic Wolf-Rayet stars Near infrared spectra of galactic and Magellanic Wolf-Rayet stars

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...81..353v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 81, no. 3, Dec. 1989, p. 353-365. Research supported by FNRS

Astronomy and Astrophysics

Astrophysics

20

Abundance, Near Infrared Radiation, Stellar Spectra, Wolf-Rayet Stars, Infrared Spectra, Magellanic Clouds, Milky Way Galaxy, Paschen Series, Stellar Winds

Scientific paper

The first part of this paper presents near infrared spectra (1650-10350 A) of galactic and mainly Magellanic Wolf Rayet Stars. The spectra are compared to the ones published previously in the 'Catalogue of near infrared spectra of southern galactic WR stars' and some peculiarities are pointed out. In the second part, the hydrogen signature in the Paschen series is discussed. For all the galactic and Magellanic objects in which such a signature could be quantified, a value of the H(+)/He(++) ratio has been derived and compared to previous estimations based on the Balmer series.

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