Clumping in the winds of O-type CSPNs

Details Clumping in the winds of O-type CSPNs Clumping in the winds of O-type CSPNs

2007-08-08

arxiv.org/abs/0708.1176v1

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures, to appear in the workshop proceedings "Clumping in Hot Star Winds", eds. W.-R. Hamann, A. Feldmeier and L.

Scientific paper

Recent studies of massive O-type stars present clear evidences of inhomogeneous and clumped winds. O-type (H-rich) central stars of planetary nebulae (CSPNs) are in some ways the low mass-low luminosity analogous of those massive stars. In this contribution, we present preliminary results of our on-going multi-wavelength (FUV, UV and optical) study of the winds of Galactic CSPNs. Particular emphasis will be given to the clumping factors derived by means of optical lines (Halpha and HeII4686) and "classic" FUV (and UV) lines.

Affiliated with

Also associated with

No associations

Rating

Clumping in the winds of O-type CSPNs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Clumping in the winds of O-type CSPNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clumping in the winds of O-type CSPNs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-416768