Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Pineault, Serge"'
Autor:
Cichowolski, Silvina, Pineault, Serge, Gamen, Roberto, Arnal, E. Marcelo, Suad, Laura A., Ortega, Martin E.
We present a study of a new molecular shell, G126.1-0.8-14, using available multiwavelegth Galactic plane surveys and optical Gemini observations. A well defined shell-like structure is observed in the CO(1--0) line emission at (l,b) = (126.1, -0.8),
Externí odkaz:
http://arxiv.org/abs/1312.4394
Autor:
Cichowolski, Silvina, Pineault, Serge
GSH91.5+2-114 is a large HI shell located in the outer Galaxy at a kinematic distance of about 15 kpc. It was first identified in the Canadian Galactic Plane Survey (CGPS) by Pineault et al. (2002) as being possibly associated with objects possessing
Externí odkaz:
http://arxiv.org/abs/1011.0922
We propose that the pulsar nebula associated with the pulsar J2229+6114 and the supernova remnant (SNR) G106.3+2.7 are the result of the same supernova explosion. The whole structure is located at the edge of an HI bubble with extended regions of mol
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106270
Autor:
Cappa, Cristina Elisabeth, Vasquez, Javier, Arnal, Edmundo Marcelo, Cichowolski, Silvina, Pineault, Serge
Publikováno v:
Mass Loss from Stars and the Evolution of Stellar Clusters
We analyze the distribution of interstellar matter in the environs of the WR stars WR 152 and WR 153ab, associated with two different ring nebulae in the H ii region Sh2-132. We have detected the radio continuum and infrared counterparts of the inner
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3498::895b85ba747ca39e9db00b1e8c49a838
http://adsabs.harvard.edu/abs/2008ASPC..388..151C
http://adsabs.harvard.edu/abs/2008ASPC..388..151C
Autor:
Cappa, Cristina Elisabeth, Vasquez, Javier, Arnal, Edmundo Marcelo, Cichowolski, Silvina, Pineault, Serge
We analyzed the distribution of the interstellar matter in the environs of the WR stars WR 152 and WR 153ab, associated with ring nebulae in the Sh2-132 HII region. Our study is based on radio data (continuum, HI, and CO(1-0) observations) and images
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3498::713be4ed50efed396a0b4d46da859c67
http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_ccappa.pdf
http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_ccappa.pdf
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We report radio continuum observations at 1465 MHz obtained with the Very Large Array (VLA) in the DnC configuration toward the ring nebulae associated with the stars WR 101 and WR 113, with resolutions of 3800 and 3000, respectively. IRAS images of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::eb09cd8a742385229a447919c1b72b78
http://iopscience.iop.org/article/10.1086/340725/meta
http://iopscience.iop.org/article/10.1086/340725/meta
Autor:
Arnal, Edmundo Marcelo, Cichowolski, Silvina, Testori, Juan Carlos, Pineault, Serge, Cappa, Cristina Elisabet
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Massive stars are known to have a profound impact on their surroundings through their high ionizing radiation, their strong stellar winds, and their eventual final explosion as supernovae. Within the area surveyed by the CGPS project there are 87 O-t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::e08e22423e85d05baad9d4aae004ec99
http://aspbooks.org/custom/publications/paper/438-0328.html
http://aspbooks.org/custom/publications/paper/438-0328.html
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
We analyse the various interstellar components of the H II region Sh2-132. The main stellar source is the double binary system that includes the Wolf–Rayet star WR 153ab. We use radio continuum images at 408 and 1420 MHz, and H I 21-cm line data ta
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::8991252f9a9598b5b0109aeee7912238
http://mnras.oxfordjournals.org/content/405/3/1976
http://mnras.oxfordjournals.org/content/405/3/1976
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Universidad Nacional de La Plata
instacron:UNLP
We report radio continuum observations at 1465 MHz obtained with the Very Large Array (VLA) in the DnC configuration toward the ring nebulae associated with the stars WR 101 and WR 113, with resolutions of ∼38″ and 30″, respectively. IRAS image
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7d5e86060944317c17bbcdebdf897e67
http://sedici.unlp.edu.ar/handle/10915/84623
http://sedici.unlp.edu.ar/handle/10915/84623
Autor:
Cazzolato, François, Pineault, Serge
Publikováno v:
Astronomical Journal; Jun2005, Vol. 129 Issue 6, p2731-2749, 19p