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

Published online by Cambridge University Press:  26 May 2016

Fabio Bresolin
Affiliation:
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
Rolf-Peter Kudritzki
Affiliation:
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
Wolfgang Gieren
Affiliation:
Universidad de Concepción, Departamento de Física, Casilla 160-C, Concepción, Chile

Abstract

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We 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 M 31 blue supergiants and with theoretical models.

Type
Part 1. Atmospheres of Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Bresolin, F., Gieren, W., Kudritzki, R.-P., Pietrzyński, G., Przybilla, N., 2002, ApJ 567, 277.CrossRefGoogle Scholar
Kudritzki, R.-P., Puls, J., Lennon, D.J., Venn, K.A., Reetz, J., Najarro, F., McCarthy, J.K., Herrero, A. 1999, A&A 350, 970.Google Scholar
Puls, J., Kudritzki, R.-P., Herrero, A., et al. 1996, A&A 305, 171.Google Scholar
Santolaya-Rey, A.E., Puls, J., Herrero, A. 1997, A&A 323, 488.Google Scholar
Zaritsky, D., Kennicutt, R.C., Huchra, J.P. 1994, ApJ 420, 87.CrossRefGoogle Scholar
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