Gamma-ray emission from massive young stellar objects: the case of IRAS 16547-4247

Details Gamma-ray emission from massive young stellar objects: the case of IRAS 16547-4247 Gamma-ray emission from massive young stellar objects: the case of IRAS 16547-4247

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33..159a&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

Hii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

The young stellar object IRAS 16547-4247, identified with a massive protostar, presents a highly collimated wind which interacts with the environments. As a result, strong shocks are formed at the jet termination point and particles are accelerated there up to relativistic energies. In the present contribution, the high-energy emission due to non-thermal interactions is calculated.

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