A Model for the Shell of HD 50138-Reference-Cited by-同舟云学术

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A Model for the Shell of HD 50138

Published:1976 Issue: Volume:70 Page:87-93
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Houziaux Léo,Andrillat Yvette

Abstract

A model for the shell star HD 50138 is inferred from the observation of the continuous spectrum from 0.14 to 10 μ.

Publisher

Cambridge University Press (CUP)

Reference11 articles.

1. The Ultra-violet Sky-Survey Telescope in the TD-1A Satellite

2. Kurucz R. L. and Peytremann E. : 1975, Special Report, Smithsonian Astrophysical Observatory.

3. Near Infra-Red Magnitudes of 248 Early-Type Emission-Line Stars and Related Objects

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1. The Complex Structure of the Mg II $\lambda\lambda$ 2795.523, 2802.698 ${\rmÅ}$ Regions of 64 Be Stars;Publications of the Astronomical Society of Japan;2007-04-25

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