The Wind Momentum-Luminosity relationship: blue supergiants in the spiral galaxy NGC 300

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dc.creatorBresolin, Fabio
dc.creatorKudritzki, Rolf-Peter
dc.creatorGieren, Wolfgang
dc.date2002-07-12
dc.date.accessioned2026-07-07T02:04:17Z
dc.date.available2026-07-07T02:04:17Z
dc.descriptionWe have carried out the wind analysis of six A-type supergiants in NGC 300. The derived Wind Momentum-Luminosity Relationship is compared with that of Galactic and M31 blue supergiants and with theoretical models.
dc.description2 pages . To appear in "A Massive Star Odyssey, from Main Sequence to Supernova", Proceedings IAU Symposium No. 212, K.A. van der Hucht, A. Herrero, & C. Esteban (eds)
dc.identifierhttps://arxiv.org/abs/astro-ph/0207266
dc.identifierhttp://arxiv.org/abs/astro-ph/0207266
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4693
dc.subjectAstrophysics
dc.titleThe Wind Momentum-Luminosity relationship: blue supergiants in the spiral galaxy NGC 300
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