Amanote Research

Amanote Research

    RegisterSign In

On the Chemical Abundances, Evolutionary Stage and Bolometric Magnitude of WR Stars

Symposium - International Astronomical Union
doi 10.1017/s0074180900028771
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1982

Authors
D. Vanbeveren
Publisher

Cambridge University Press (CUP)


Related search

Chemical Abundances of Fast-Rotating Massive Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Chemical Abundances of Hot Post-Agb Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

The Bolometric Luminosities of Stars

Symposium - International Astronomical Union
1997English

Atmospheric Parameters and Chemical Abundances for Herbig Ae Stars

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Chemical Abundances of Distant Extremely Metal-Poor Unevolved Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Chemical Imprints in Atmospheric Abundances in Planet- Hosting Stars

Odessa Astronomical Publications
2019English

Comparing Chemical Abundances of the Damped Lyα Systems and Metal-Poor Stars

Highlights of Astronomy
2005English

Hydrodynamic Model Atmospheres for WR Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

General Discussion on Chemical Abundances

Symposium - International Astronomical Union
2001English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy