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A FUSE View of Winds from the Central Stars of Planetary Nebulae

Published online by Cambridge University Press:  02 January 2013

Martín A. Guerrero ,
Gerardo Ramos-Larios  and
Derck Massa
Martín A. Guerrero*
Affiliation:
Instituto de Astrofísica de Andalucía, CSIC. Camino Bajo de Huétor 50, E–18008 Granada, Spain
Gerardo Ramos-Larios
Affiliation:
Instituto de Astrofísica de Andalucía, CSIC. Camino Bajo de Huétor 50, E–18008 Granada, Spain Instituto de Astronomía y Meteorología, Av. Vallarta No. 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, Mexico
Derck Massa
Affiliation:
NASA Goddard Space Flight Center, Mail Code 130, Greenbelt, Maryland 20771, USA, SGT Inc.
*
DCorresponding author. Email: mar@iaa.es
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Abstract

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Since the IUE satellite produced a vast collection of high-resolution UV spectra of the central stars of planetary nebulae (CSPNe), there has not been any further systematic study of the stellar winds of these stars. The high spectral resolution, sensitivity and large number of archival observations in the FUSE archive allow the study of the stellar winds of CSPNe in the far-UV domain where lines of species spanning a wide excitation range can be observed. We present here a preliminary analysis of the P Cygni profiles of a sample of ∼60 CSPNe observed by FUSE. P Cygni profiles providing evidence for fast stellar winds with velocities between 200 and 4300 km s−1 have been found in 40 CSPNe. In many cases, this is the first time that fast stellar winds have been reported for these planetary nebulae (PNe). A detailed study of these far-UV spectra is on-going.

Keywords

line: profilesplanetary nebulaestars: windsoutflowsultraviolet: stars
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 27 , Issue 2 , 2010 , pp. 210 - 213
Copyright
Copyright © Astronomical Society of Australia 2010

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