Quantitative analysis of WC stars: constraints on neon abundances from ISO-SWS spectroscopy
Open Access
- 21 June 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 315 (2) , 407-422
- https://doi.org/10.1046/j.1365-8711.2000.03399.x
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This publication has 46 references indexed in Scilit:
- Radio Continuum Measurements of Southern Early‐Type Stars. III. Nonthermal Emission from Wolf‐Rayet StarsThe Astrophysical Journal, 1999
- Quantitative classification of WC and WO starsMonthly Notices of the Royal Astronomical Society, 1998
- Multifrequency observations of the Wolf-Rayet star WR 146: another colliding-wind binary?Monthly Notices of the Royal Astronomical Society, 1996
- An infrared view of Wolf-Rayet WC subtypes - II. Abundances in stratified windsMonthly Notices of the Royal Astronomical Society, 1992
- An infrared view of Wolf-Rayet WC subtypes - I. Line identification and spectral characteristicsMonthly Notices of the Royal Astronomical Society, 1991
- The relationship between infrared, optical, and ultraviolet extinctionThe Astrophysical Journal, 1989
- The determination of wind terminal velocities and ionic abundances from infrared fine-structure lines: the WC8 component of VelorumMonthly Notices of the Royal Astronomical Society, 1988
- Infrared speckle interferometry and imaging of several OH/IR starsThe Astrophysical Journal, 1987
- The DBA white dwarf stars in the Palomar-Green sampleThe Astrophysical Journal, 1987
- Mass loss from very luminous OB stars and the Cygnus superbubbleThe Astrophysical Journal, 1981