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A compact nebulosity surrounding the peculiar blue emission-line supergiant HD 37836 of the LMC

Published online by Cambridge University Press:  04 August 2017

O. Stahl  and
B. Wolf
O. Stahl
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-8046 Garching b. München, FRG
B. Wolf
Affiliation:
Landessternwarte Heidelberg D-6900 Heidelberg-Königstuhl, FRG

Abstract

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HD 37836 (= R 123; Feast et al., 1960) is one of the brightest slightly variable (V ≃ 10.5–10.7; Stahl et al., 1984) emission-line stars of the LMC. Since it is also likely to be a hot star (see below) it is also bolometrically very bright (Mbol ≤ −11).

Type
Mass Loss from Hot Stars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 441 - 442
Copyright
Copyright © Reidel 1987 

References

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