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The Near Infrared Properties of Selected WN Stars in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

N. Panagia ,
E.G. Tanzi  and
M. Tarenghi
N. Panagia
Affiliation:
(1)Istituto di Radioastronomia, CNR, Bologna
E.G. Tanzi
Affiliation:
(2)Istituto di Fisica Cosmica, CNR, Milano
M. Tarenghi
Affiliation:
(3)European Southern Observatory, Garching b. München

Extract

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We report here on preliminary infrared photometry of six WN stars in the Large Magellanic Cloud. Besides R136, the central object of the 30 Doradus Nebula, the sample includes three stars (R139, R140, R145) located near the center of the region (within ∼ 1 arcmin) and two more stars (R144, R147) at a distance of ∼ 5 arcmin from R136.

Type
SESSION 3 — MASS-LOSS FROM WR STARS: OBSERVATIONS AND THEORY
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 231 - 235
Copyright
Copyright © Reidel 1982 

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