2011
DOI: 10.1051/0004-6361/201116580
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A study of the association ofFermisources with massive young galactic objects

Abstract: 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 associat… Show more

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Cited by 15 publications
(15 citation statements)
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“…The following sections in this paper are devoted to this purpose by assessing the observational evidence and theoretical expectations in the Mon R2 case. The present work complements other efforts to identify massive YSOs as potential counterparts of some galactic Fermi sources (Munar-Adrover et al 2011). …”
Section: Introductionsupporting
confidence: 58%
“…The following sections in this paper are devoted to this purpose by assessing the observational evidence and theoretical expectations in the Mon R2 case. The present work complements other efforts to identify massive YSOs as potential counterparts of some galactic Fermi sources (Munar-Adrover et al 2011). …”
Section: Introductionsupporting
confidence: 58%
“…Araudo et al 2007;Bosch-Ramon et al 2010;Munar-Adrover et al 2011). The organisation of the paper is the following.…”
Section: Introductionmentioning
confidence: 99%
“…Several approaches to attack this problem on both statistical grounds (e.g., Munar-Adrover et al 2011;Ackermann et al 2012b;D'Abrusco et al 2013) and observational grounds (e.g., Mirabal & Halpern 2009;Shaw et al 2012Shaw et al , 2013 were applied in recent years.…”
Section: Introductionmentioning
confidence: 99%