A CGPS view of the ISM towards HD 192281
- Autores
- Arnal, Edmundo Marcelo; Cichowolski, Silvina; Testori, Juan Carlos; Pineault, Serge; Cappa, Cristina Elisabet
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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-type stars and 36 Galactic Wolf-Rayet stars. Therefore, the CGPS is an ideal database to study, in a large number of stellar targets, the interaction of massive stars (and their descendants) with their surroundings. In this paper we report on a study carried out towards the massive stars HD 192281. A shell-like structure, detectable at radio continuum, infrared and neutral hydrogen wavelengths, is found to be associated with this star.
Trabajo publicado en Kothes, R.; Landecker, T. L.; Willis, A. G. (2011). The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey. ASP Conference Series, vol. 438. ISBN: 978-1-58381-756-8.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Astronomía
Física
Massive stars
Wolf-rayet stars
High ionizing radiation
HD 192281 (estrella) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/102530
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A CGPS view of the ISM towards HD 192281Arnal, Edmundo MarceloCichowolski, SilvinaTestori, Juan CarlosPineault, SergeCappa, Cristina ElisabetAstronomíaFísicaMassive starsWolf-rayet starsHigh ionizing radiationHD 192281 (estrella)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-type stars and 36 Galactic Wolf-Rayet stars. Therefore, the CGPS is an ideal database to study, in a large number of stellar targets, the interaction of massive stars (and their descendants) with their surroundings. In this paper we report on a study carried out towards the massive stars HD 192281. A shell-like structure, detectable at radio continuum, infrared and neutral hydrogen wavelengths, is found to be associated with this star.Trabajo publicado en Kothes, R.; Landecker, T. L.; Willis, A. G. (2011). <i>The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey</i>. ASP Conference Series, vol. 438. ISBN: 978-1-58381-756-8.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2011info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf328-334http://sedici.unlp.edu.ar/handle/10915/102530enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/6256info:eu-repo/semantics/altIdentifier/url/http://aspbooks.org/custom/publications/paper/438-0328.htmlinfo:eu-repo/semantics/altIdentifier/issn/0004-6280info:eu-repo/semantics/altIdentifier/hdl/11336/6256info: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:UNLP2025-09-29T11:20:15Zoai:sedici.unlp.edu.ar:10915/102530Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:20:16.227SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A CGPS view of the ISM towards HD 192281 |
| title |
A CGPS view of the ISM towards HD 192281 |
| spellingShingle |
A CGPS view of the ISM towards HD 192281 Arnal, Edmundo Marcelo Astronomía Física Massive stars Wolf-rayet stars High ionizing radiation HD 192281 (estrella) |
| title_short |
A CGPS view of the ISM towards HD 192281 |
| title_full |
A CGPS view of the ISM towards HD 192281 |
| title_fullStr |
A CGPS view of the ISM towards HD 192281 |
| title_full_unstemmed |
A CGPS view of the ISM towards HD 192281 |
| title_sort |
A CGPS view of the ISM towards HD 192281 |
| dc.creator.none.fl_str_mv |
Arnal, Edmundo Marcelo Cichowolski, Silvina Testori, Juan Carlos Pineault, Serge Cappa, Cristina Elisabet |
| author |
Arnal, Edmundo Marcelo |
| author_facet |
Arnal, Edmundo Marcelo Cichowolski, Silvina Testori, Juan Carlos Pineault, Serge Cappa, Cristina Elisabet |
| author_role |
author |
| author2 |
Cichowolski, Silvina Testori, Juan Carlos Pineault, Serge Cappa, Cristina Elisabet |
| author2_role |
author author author author |
| dc.subject.none.fl_str_mv |
Astronomía Física Massive stars Wolf-rayet stars High ionizing radiation HD 192281 (estrella) |
| topic |
Astronomía Física Massive stars Wolf-rayet stars High ionizing radiation HD 192281 (estrella) |
| dc.description.none.fl_txt_mv |
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-type stars and 36 Galactic Wolf-Rayet stars. Therefore, the CGPS is an ideal database to study, in a large number of stellar targets, the interaction of massive stars (and their descendants) with their surroundings. In this paper we report on a study carried out towards the massive stars HD 192281. A shell-like structure, detectable at radio continuum, infrared and neutral hydrogen wavelengths, is found to be associated with this star. Trabajo publicado en Kothes, R.; Landecker, T. L.; Willis, A. G. (2011). <i>The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey</i>. ASP Conference Series, vol. 438. ISBN: 978-1-58381-756-8. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
| description |
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-type stars and 36 Galactic Wolf-Rayet stars. Therefore, the CGPS is an ideal database to study, in a large number of stellar targets, the interaction of massive stars (and their descendants) with their surroundings. In this paper we report on a study carried out towards the massive stars HD 192281. A shell-like structure, detectable at radio continuum, infrared and neutral hydrogen wavelengths, is found to be associated with this star. |
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2011 |
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2011 |
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eng |
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