Clumping in Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics

Details Clumping in Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics Clumping in Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cihw.conf..247l&link_type=abstract

Clumping in hot-star winds : proceedings of an international workshop held in Potsdam, Germany, 18. - 22. June 2007. Hamann, Wol

Other

1

Scientific paper

The mass loss rates and other parameters for a large sample of Galactic WN stars have been revised by Hamann et al. (2006), using the most up-to date Potsdam Wolf-Rayet (PoWR) model atmospheres. For a sub-sample of these stars exist measurements of their radio free-free emission. After harmonizing the adopted distance and terminal wind velocities, we compare the mass loss rates obtained from the two diagnostics. The differences are discussed as a possible consequence of different clumping contrast in the line-forming and radio-emitting regions.

Affiliated with

Also associated with

No associations

Rating

Clumping in Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics 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 Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clumping in Galactic WN stars : a comparison of mass loss rates from UV/optical & radio diagnostics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1340557