Properties of massive Population III and metal-poor stars

Details Properties of massive Population III and metal-poor stars Properties of massive Population III and metal-poor stars

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..211s&link_type=abstract

Highlights of Astronomy, Volume 14, p. 211-211

Astronomy and Astrophysics

Astronomy

Galaxies:High-Redshift, Stars: Population Iii, Stars: General

Scientific paper

We review the properties of massive Population III and very metal-poor stars, including briefly their formation, IMF, their main sequence evolution, possible mass loss mechanisms, atmosphere modeling etc. For detailed predictions concerning the properties of these stars we refer to Schaerer (2002) and Schaerer (2002) and references therein. Extending these calculations, Schaerer (2007) present new calculations concerning the ionizing power, Ly-α strength and related properties for different metallicities as well as for a range of power-law and log-normal IMFs. For illustrations from these studies see the Figures below. New detailed calibrations for solar metallicity O-type stars have recently been presented by Martins et al. (2005).

Affiliated with

Also associated with

No associations

Rating

Properties of massive Population III and metal-poor 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 Properties of massive Population III and metal-poor stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of massive Population III and metal-poor stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974572