A DRAO and VLA investigation of the environment of WR 130
- Autores
- Cichowolski, Silvina; Pineault, Serge; Arnal, Edmundo Marcelo; Testori, Juan Carlos; Goss, W. M.; Cappa, Cristina Elisabet
- Año de publicación
- 2001
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed using the Very Large Array in the DnC and D configurations.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
astrofísica - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-nd/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/2054
Ver los metadatos del registro completo
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A DRAO and VLA investigation of the environment of WR 130Cichowolski, SilvinaPineault, SergeArnal, Edmundo MarceloTestori, Juan CarlosGoss, W. M.Cappa, Cristina ElisabetCiencias AstronómicasastrofísicaThe environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed using the Very Large Array in the DnC and D configurations.Facultad de Ciencias Astronómicas y Geofísicas2001info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1938-1953http://sedici.unlp.edu.ar/handle/10915/2054enginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1086/323092/metainfo:eu-repo/semantics/altIdentifier/issn/1538-3881info:eu-repo/semantics/altIdentifier/doi/10.1086/323092info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-12-23T10:51:32Zoai:sedici.unlp.edu.ar:10915/2054Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-12-23 10:51:33.093SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A DRAO and VLA investigation of the environment of WR 130 |
| title |
A DRAO and VLA investigation of the environment of WR 130 |
| spellingShingle |
A DRAO and VLA investigation of the environment of WR 130 Cichowolski, Silvina Ciencias Astronómicas astrofísica |
| title_short |
A DRAO and VLA investigation of the environment of WR 130 |
| title_full |
A DRAO and VLA investigation of the environment of WR 130 |
| title_fullStr |
A DRAO and VLA investigation of the environment of WR 130 |
| title_full_unstemmed |
A DRAO and VLA investigation of the environment of WR 130 |
| title_sort |
A DRAO and VLA investigation of the environment of WR 130 |
| dc.creator.none.fl_str_mv |
Cichowolski, Silvina Pineault, Serge Arnal, Edmundo Marcelo Testori, Juan Carlos Goss, W. M. Cappa, Cristina Elisabet |
| author |
Cichowolski, Silvina |
| author_facet |
Cichowolski, Silvina Pineault, Serge Arnal, Edmundo Marcelo Testori, Juan Carlos Goss, W. M. Cappa, Cristina Elisabet |
| author_role |
author |
| author2 |
Pineault, Serge Arnal, Edmundo Marcelo Testori, Juan Carlos Goss, W. M. Cappa, Cristina Elisabet |
| author2_role |
author author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas astrofísica |
| topic |
Ciencias Astronómicas astrofísica |
| dc.description.none.fl_txt_mv |
The environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed using the Very Large Array in the DnC and D configurations. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
The environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed using the Very Large Array in the DnC and D configurations. |
| publishDate |
2001 |
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2001 |
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http://sedici.unlp.edu.ar/handle/10915/2054 |
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eng |
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eng |
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