Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..183p&link_type=abstract
HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 183-190 (2001).
Astronomy and Astrophysics
Astronomy
3
Pre-Main Sequence Objects, Young Stellar Objects And Protostars, Origin, Formation, Evolution, Age, And Star Formation, Radiation Mechanisms, Polarization
Scientific paper
Star-formation regions are the most active sites in our Galaxy. The combined activity of their stellar population is in a position to produce detectable amount of gamma rays, but the observational evidence for high-energy emission from specific early-type stars has remained rather elusive till now. After having summarized the lessons from large-scale studies relevant to the production of gamma rays in star-formation regions, the paper discusses the contribution of young stellar objects in the framework of their protoscalar activity as well as the high-energy emission from massive early-type mass-losing stars. .
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