The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum

Details The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138...25l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, p. 25-35.

Astronomy and Astrophysics

Astrophysics

24

Early Stars, Infrared Spectra, Radio Spectra, Stellar Mass Ejection, Stellar Winds, Stellar Coronas, Stellar Models, Stellar Spectra, Stellar Temperature, Temperature Distribution

Scientific paper

The effect of different temperature structures and of clumping and hot blobs in stellar winds on the infrared and radio excess is studied. It is shown that the presence of a corona can lead to either an increase or a decrease of the IR excess, depending on the theoretical depth of the corona. In the case of hot blobs or hot filaments, the excess flux may also be either higher or lower than in a comparable isothermal wind without clumping. The excess flux can be simply calculated from the predicted excess flux of homogeneous isothermal wind models by applying a correction factor to the optical depth scale and a correction factor to the source function. For a wind with hot and cold blobs of the same density, the excess flux is smaller than from a comparable star with a homogeneous wind with the same mass loss rate and velocity law.

Affiliated with

Also associated with

No associations

Rating

The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum 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 The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The infrared and radio spectrum of early type stars with mass loss. III - The effect of coronae, hot blobs and clumping on the IR and radio spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1389246