The evolution of massive stars - an observational viewpoint

Details The evolution of massive stars - an observational viewpoint The evolution of massive stars - an observational viewpoint

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...26..331h&link_type=abstract

Space Science Reviews, vol. 26, July 1980, p. 331-345.

Computer Science

3

B Stars, O Stars, Stellar Evolution, Stellar Luminosity, Stellar Mass Ejection, Supermassive Stars, Abundance, Binary Stars, Mass Flow Rate, Stellar Temperature, Stellar Winds

Scientific paper

A review of observationally deduced values of the masses, mass-loss rates, temperatures, luminosities and element abundances for the most massive stars is presented. The stars considered range from 30 to over 100 solar masses. Further, their luminosities are 10 to the 5th to 10 to the 6.3 solar luminosities and they are of types O and B. The calculated quantities are compared with theoretical calculations and discussed in terms of present understanding of their evolutions.

Affiliated with

Also associated with

No associations

Rating

The evolution of massive stars - an observational viewpoint 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 evolution of massive stars - an observational viewpoint, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of massive stars - an observational viewpoint will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-804787