Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Paron, Sergio"'
Autor:
Peña, M. Celis, Paron, Sergio
In recent works, through observations of molecular lines, we found that the supernova remnant (SNR) G18.8+0.3 is interacting with a molecular cloud towards its southern edge. Also it has been proven the presence of several neighboring HII regions ver
Externí odkaz:
http://arxiv.org/abs/1606.00084
Autor:
Suárez, Alejandra E., Combi, Jorge A., Albacete-Colombo, Juan F., Paron, Sergio, García, Federico, Miceli, Marco
We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 through an exhaustive analysis of XMM-Netwon observations with complementary infrared observations. We characterize and discuss the origin of the observed X-ray
Externí odkaz:
http://arxiv.org/abs/1510.01215
Aims: We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high energy counterpart of the radio nebula and to find evidence of interaction between the shock front and the interstellar medium. Methods: We used Chandra
Externí odkaz:
http://arxiv.org/abs/1304.3058
Autor:
Paron, Sergio, Weidmann, Walter
Using data from large-scale surveys: 2MASS, GLIMPSE, MIPSGAL, VGPS, GRS, and IPHAS, we performed a multiwavelength study of the ISM in a region of about 20' x 20' towards the molecular cloud G35.2-0.74. Additionally, the Ap 2-1 nebula, that is seen i
Externí odkaz:
http://arxiv.org/abs/1007.0724
Akademický článek
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Autor:
Pe��a, M. Celis, Paron, Sergio
In recent works, through observations of molecular lines, we found that the supernova remnant (SNR) G18.8+0.3 is interacting with a molecular cloud towards its southern edge. Also it has been proven the presence of several neighboring HII regions ver
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88d1c16620b8ca0ff2d584ca7900ab99
http://arxiv.org/abs/1606.00084
http://arxiv.org/abs/1606.00084
Autor:
Su��rez, Alejandra E., Combi, Jorge A., Albacete-Colombo, Juan F., Paron, Sergio, Garc��a, Federico, Miceli, Marco
We present an X-ray analysis of the central region of supernova remnant (SNR) G332.5-5.6 through an exhaustive analysis of XMM-Netwon observations with complementary infrared observations. We characterize and discuss the origin of the observed X-ray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46fb549c7df42c595acc71da2be39095
http://arxiv.org/abs/1510.01215
http://arxiv.org/abs/1510.01215
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We analize the 12CO emission towards the brightest X-ray knot in the supernova remnant (SNR) Puppis A. The observations were performed with the SEST telescope in the 12CO J=1--0 and 2--1 lines (beams of 45" and 23" respectively). We discovered a comp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0e223eadc20e5e47c4348baa1ced3fe5
http://www.astronomiaargentina.org.ar/uploads/docs/baaa_50.pdf
http://www.astronomiaargentina.org.ar/uploads/docs/baaa_50.pdf
Autor:
Paron, Sergio Ariel, Reynoso, Estela Marta, Dubner, Gloria Mabel, Castelletti, Gabriela Marta
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
RCW 103 is a shell type supernova remnant (SNR) that, according to near infrared observations, is interacting with a molecular cloud, specially to the south. In this paper we report on the study of the interstellar medium in an extended region toward
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::6953b4184df22d85aa12083c590f3711
http://www.astronomiaargentina.org.ar/uploads/docs/baaa_47.pdf
http://www.astronomiaargentina.org.ar/uploads/docs/baaa_47.pdf
Akademický článek
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