Fermi sources with massive YSO associations (Munar-Adrover+, 2011)

Details Fermi sources with massive YSO associations (Munar-Adrover+, 2011) Fermi sources with massive YSO associations (Munar-Adrover+, 2011)

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35309072m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/530/A72. Originally published in: 2011A&A...530A..72M

Mathematics

Probability

Gamma Rays, Ysos

Scientific paper

Massive protostars have associated bipolar outflows that can produce strong shocks when they interact with the surrounding medium. At these shocks, particles can be accelerated up to relativistic energies. Relativistic electrons and protons can then produce gamma-ray emission, as some theoretical models predict. To identify young galactic objects that may emit gamma rays, we crossed the Fermi First Year Catalog with some catalogs of known massive young stellar objects (MYSOs), early type stars, and OB associations, and we implemented Monte Carlo simulations to find the probability of chance coincidences. We obtained a list of massive MYSOs that are spatially coincident with Fermi sources.
(4 data files).

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