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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
Abstract
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