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dc.date.accessioned 2019-10-01T16:36:22Z
dc.date.available 2019-10-01T16:36:22Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82416
dc.description.abstract Massive protostars have associated bipolar outflows which can produce strong shocks when interact with the surrounding medium. Some theoretical models predict that particle acceleration at relativistic velocities can occur leading to gamma ray emission. In order to identify young stellar objects (YSO) that might emit gamma rays, we have crossed the Fermi First Year Catalog with catalogs of known YSOs, obtaining a set of candidates by spatial correlation. We have conducted Montecarlo simulations to find the probability of chance coincidence. Our results indicate that ∼70% of the candidates should be gamma-ray sources with a confidence of ∼5ρ. σ International Astronomical Union 2011. en
dc.format.extent 406-407 es
dc.language en es
dc.subject Gamma rays: observations es
dc.subject ISM: jets and outflows es
dc.subject Stars: early-type es
dc.title Exploring the association of Fermi sources with Young Stellar Objects en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-84882781779 es
sedici.identifier.other doi:10.1017/S1743921310016509 es
sedici.identifier.issn 17439213 es
sedici.creator.person Munar-Adrover, P. es
sedici.creator.person Paredes, J. M. es
sedici.creator.person Romero, Gustavo Esteban es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto Argentino de Radioastronomía es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 275 (Buenos Aires, Argentina, 13-17 September, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. S275 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)