The relation between apparent temperature and mass-loss rate in hypergiant eruptions

Details The relation between apparent temperature and mass-loss rate in hypergiant eruptions The relation between apparent temperature and mass-loss rate in hypergiant eruptions

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...317..760d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 317, June 15, 1987, p. 760-764.

Astronomy and Astrophysics

Astrophysics

86

Stellar Mass Ejection, Stellar Temperature, Stellar Winds, Supergiant Stars, Variable Stars, Blue Stars, Stellar Models

Scientific paper

A simplified opaque wind model is used to estimate the emergent radiation temperature as a function of mass loss rate for giant eruptions of luminous blue variable stars. It is conjectured that this relation applies to the pseudo-photospheres of S Dor, R127, and P Cyg during their major outbursts, and to the wind itself of Eta Car during a giant outburst.

Affiliated with

Also associated with

No associations

Rating

The relation between apparent temperature and mass-loss rate in hypergiant eruptions 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 relation between apparent temperature and mass-loss rate in hypergiant eruptions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The relation between apparent temperature and mass-loss rate in hypergiant eruptions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1814071