Skip to main content Accessibility help
×
Home

DIVISION IV / WORKING GROUP on MASSIVE STARS

  • Joachim Puls, Claus Leitherer, Stan Owocki, Paul Crowther, Margaret Hanson, Artemio Herrero, Norbert Langer, Stan Owocki, Gregor Rauw, Nicole St-Louis and Richard Townsend...

Extract

Our Working Group (WG) studies massive, luminous stars, both individually and in resolved and unresolved populations, with historical focus on early-type (OB) stars, A-supergiants, and Wolf-Rayet stars. Our group also studies lower mass stars (e.g., central stars of planetary nebulae and their winds) which display features similar or related to those present in massive stars, and thus may improve our understanding of the physical processes occurring in massive stars. In recent years, massive red supergiants that evolve from hot stars have been included into our activities as well. We emphasize the role of massive stars in other branches of astrophysics, particularly regarding the First Stars, long duration Gamma-Ray bursts, formation of massive stars and their feedback on star formation in general, pulsations of massive stars, and starburst galaxies.

Copyright

References

Hide All
Crowther, P. A., Schnurr, O., Hirschi, R., et al. , 2010, MNRAS, 408, 731
Gal-Yam, A., Mazzali, P., Ofek, E. O., et al. , 2009, Nature, 462, 624
Leitherer, C., Bennett, P., Morris, P. & van Loon, J. (editors) 2010, Astronomical Society of the Pacific Conference Series, 425
MathJax
MathJax is a JavaScript display engine for mathematics. For more information see http://www.mathjax.org.

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed