Hostname: page-component-7bb8b95d7b-l4ctd Total loading time: 0 Render date: 2024-09-13T04:07:43.789Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar winds in central stars of LMC planetary nebulae

Published online by Cambridge University Press:  15 December 2006

Anabel Arrieta ,
L. Stanghellini  and
L. Georgiev
Anabel Arrieta
Affiliation:
Depto. Física y Matemáticas, Univ. Iberoamericana, Av. Prol. Paseo de la Reforma 880, Lomas de Santa Fe, México, D.F. C.P. 01210, México email: [email protected]
L. Stanghellini
Affiliation:
NOAO, Tucson AZ, USA
L. Georgiev
Affiliation:
Instituto Astronomía UNAM, México, D.F.
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this work we investigate the relation between wind momentum $\Pi$ and the luminosity of the CSPNs in the LMC taking advantage of the less uncertain distances to these objects. We show that these winds obey the same relation as the Galactic O stars and therefore have the same physics.

Keywords

Central Star Planetary NebulaStellar WindsLMC Planetary NebulaeWind momentum relation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 359 - 360
Copyright
© 2006 International Astronomical Union