A search for young stellar objects as possible counterparts of Fermi sources
- Autores
- Munar Adrover, P.; Paredes, Josep M.; Romero, Gustavo Esteban
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Massive protostars have associated bipolar outflows which can produce strong shocks when interact with the surrounding medium. Some theoretical models predict that, under some conditions, 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 Monte Carlo 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 ∼ 5σ.
Instituto Argentino de Radioastronomía - Materia
- Astronomía
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
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- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/141460
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A search for young stellar objects as possible counterparts of Fermi sourcesMunar Adrover, P.Paredes, Josep M.Romero, Gustavo EstebanAstronomíaMassive protostars have associated bipolar outflows which can produce strong shocks when interact with the surrounding medium. Some theoretical models predict that, under some conditions, 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 Monte Carlo 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 ∼ 5σ.Instituto Argentino de Radioastronomía2011-06-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/141460enginfo:eu-repo/semantics/altIdentifier/doi/10.22323/1.123.0256info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:13:02Zoai:sedici.unlp.edu.ar:10915/141460Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:13:02.547SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A search for young stellar objects as possible counterparts of Fermi sources |
| title |
A search for young stellar objects as possible counterparts of Fermi sources |
| spellingShingle |
A search for young stellar objects as possible counterparts of Fermi sources Munar Adrover, P. Astronomía |
| title_short |
A search for young stellar objects as possible counterparts of Fermi sources |
| title_full |
A search for young stellar objects as possible counterparts of Fermi sources |
| title_fullStr |
A search for young stellar objects as possible counterparts of Fermi sources |
| title_full_unstemmed |
A search for young stellar objects as possible counterparts of Fermi sources |
| title_sort |
A search for young stellar objects as possible counterparts of Fermi sources |
| dc.creator.none.fl_str_mv |
Munar Adrover, P. Paredes, Josep M. Romero, Gustavo Esteban |
| author |
Munar Adrover, P. |
| author_facet |
Munar Adrover, P. Paredes, Josep M. Romero, Gustavo Esteban |
| author_role |
author |
| author2 |
Paredes, Josep M. Romero, Gustavo Esteban |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Astronomía |
| topic |
Astronomía |
| dc.description.none.fl_txt_mv |
Massive protostars have associated bipolar outflows which can produce strong shocks when interact with the surrounding medium. Some theoretical models predict that, under some conditions, 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 Monte Carlo 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 ∼ 5σ. Instituto Argentino de Radioastronomía |
| description |
Massive protostars have associated bipolar outflows which can produce strong shocks when interact with the surrounding medium. Some theoretical models predict that, under some conditions, 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 Monte Carlo 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 ∼ 5σ. |
| publishDate |
2011 |
| dc.date.none.fl_str_mv |
2011-06-06 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/141460 |
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| dc.language.none.fl_str_mv |
eng |
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eng |
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info:eu-repo/semantics/altIdentifier/doi/10.22323/1.123.0256 |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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