The star forming region Monoceros R2 as a gamma-ray source

Context. After the release of the gamma-ray source catalog produced by the <i>Fermi</i> satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supe...

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Autores principales: Martí, J., Luque Escamilla, P. L., Muñoz Arjonilla, A. J., Sánchez Ayaso, E., Munar Adrover, P., Sánchez Sutil, J. R., Romero, Gustavo Esteban, Paredes, J. M., Combi, Jorge Ariel
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85186
Aporte de:
id I19-R120-10915-85186
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Gamma rays: stars
Radio continuum: stars
Stars: flare
Stars: massive
Stars: protostars
X-rays: stars
spellingShingle Ciencias Astronómicas
Gamma rays: stars
Radio continuum: stars
Stars: flare
Stars: massive
Stars: protostars
X-rays: stars
Martí, J.
Luque Escamilla, P. L.
Muñoz Arjonilla, A. J.
Sánchez Ayaso, E.
Munar Adrover, P.
Sánchez Sutil, J. R.
Romero, Gustavo Esteban
Paredes, J. M.
Combi, Jorge Ariel
The star forming region Monoceros R2 as a gamma-ray source
topic_facet Ciencias Astronómicas
Gamma rays: stars
Radio continuum: stars
Stars: flare
Stars: massive
Stars: protostars
X-rays: stars
description Context. After the release of the gamma-ray source catalog produced by the <i>Fermi</i> satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood. Aims. The aim of this paper is to assess the possibility of the <i>Fermi</i> gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2. Methods. A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios. Results. We confirm the 2FGL J0607.5-0618c detection with improved confidence over the <i>Fermi</i> two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source.
format Articulo
Articulo
author Martí, J.
Luque Escamilla, P. L.
Muñoz Arjonilla, A. J.
Sánchez Ayaso, E.
Munar Adrover, P.
Sánchez Sutil, J. R.
Romero, Gustavo Esteban
Paredes, J. M.
Combi, Jorge Ariel
author_facet Martí, J.
Luque Escamilla, P. L.
Muñoz Arjonilla, A. J.
Sánchez Ayaso, E.
Munar Adrover, P.
Sánchez Sutil, J. R.
Romero, Gustavo Esteban
Paredes, J. M.
Combi, Jorge Ariel
author_sort Martí, J.
title The star forming region Monoceros R2 as a gamma-ray source
title_short The star forming region Monoceros R2 as a gamma-ray source
title_full The star forming region Monoceros R2 as a gamma-ray source
title_fullStr The star forming region Monoceros R2 as a gamma-ray source
title_full_unstemmed The star forming region Monoceros R2 as a gamma-ray source
title_sort star forming region monoceros r2 as a gamma-ray source
publishDate 2013
url http://sedici.unlp.edu.ar/handle/10915/85186
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