IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars

Details IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..217n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 217-226

Astronomy and Astrophysics

Astronomy

4

Infrared Spectra, Radio Emission, Stellar Mass, Stellar Physics, Stellar Winds, Wolf-Rayet Stars, Density (Mass/Volume), Infrared Astronomy, Line Spectra, Mass Ratios, Radio Astronomy, Stellar Models, Wind Velocity

Scientific paper

Spherically-symmetric homogeneous (smooth) wind models predict smaller than the observed IR-fluxes and in many cases also smaller than the observed fluxes of HeI lines (in some cases also of HeII lines) if matter density is calibrated through the observed radio-fluxes. These discrepancies can be removed by clumped wind models. The mass loss rates determined for Wolf-Rayet stars by standard techniques through the radio-flux values seem to be the overestimates up to 1.1-2.5 times.

Affiliated with

Also associated with

No associations

Rating

IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars 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 IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IR-and radio-fluxes from smooth and clumped wind models of Wolf-Rayet stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1021721