The H I supershell GS 118+01-44 and its role in the interstellar medium
- Autores
- Suad, Laura Andrea; Cichowolski, Silvina; Noriega Crespo, A.; Arnal, Edmundo Marcelo; Testori, Juan Carlos; Flagey, N.
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Aims. We carry out a multiwavelength study to characterize the H i supershell designated GS 118+01−44, and to analyse its possible origin. Methods. A multiwavelength study has been carried out to study the supershell and its environs. We performed an analysis of the H i, CO, radio continuum, and infrared emission distributions. Results. The Canadian Galactic Plane Survey (CGPS) H i data reveals that GS 118+01−44 is centred at (l,b) = (117°̣7, 1°̣4) with a systemic velocity of −44.3 km s-1. According to Galactic rotation models this structure is located at 3.0 ± 0.6 kpc from the Sun. There are several H ii regions and three supernova remnants (SNRs) catalogued in the region. On the other hand, the analysis of the temperature spectral index distribution shows that in the region there is a predominance of non-thermal emission. Infrared emission shows that cool temperatures dominate the area of the supershell. Concerning the origin of the structure, we found that even though several OB stars belonging to Cas OB5 are located in the interior of GS 118+01−44, an analysis of the energy injected by these stars through their stellar winds indicates that they do not have sufficient energy to create GS 118+01−44. Therefore, an additional energy source is needed to explain the genesis of GS 118+01−44. On the other hand, the presence of several H ii regions and young stellar object candidates in the edges of GS 118+01−44 shows that the region is still active in forming new stars.
Fil: Suad, Laura Andrea. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Cichowolski, Silvina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Noriega Crespo, A.. Space Telescope Science Institute; Estados Unidos
Fil: Arnal, Edmundo Marcelo. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Flagey, N.. Space Telescope Science Institute; Estados Unidos - Materia
-
ISM: bubbles
ISM: kinematics and dynamics
HII regions
stars: formation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/21538
Ver los metadatos del registro completo
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The H I supershell GS 118+01-44 and its role in the interstellar mediumSuad, Laura AndreaCichowolski, SilvinaNoriega Crespo, A.Arnal, Edmundo MarceloTestori, Juan CarlosFlagey, N.ISM: bubblesISM: kinematics and dynamicsHII regionsstars: formationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Aims. We carry out a multiwavelength study to characterize the H i supershell designated GS 118+01−44, and to analyse its possible origin. Methods. A multiwavelength study has been carried out to study the supershell and its environs. We performed an analysis of the H i, CO, radio continuum, and infrared emission distributions. Results. The Canadian Galactic Plane Survey (CGPS) H i data reveals that GS 118+01−44 is centred at (l,b) = (117°̣7, 1°̣4) with a systemic velocity of −44.3 km s-1. According to Galactic rotation models this structure is located at 3.0 ± 0.6 kpc from the Sun. There are several H ii regions and three supernova remnants (SNRs) catalogued in the region. On the other hand, the analysis of the temperature spectral index distribution shows that in the region there is a predominance of non-thermal emission. Infrared emission shows that cool temperatures dominate the area of the supershell. Concerning the origin of the structure, we found that even though several OB stars belonging to Cas OB5 are located in the interior of GS 118+01−44, an analysis of the energy injected by these stars through their stellar winds indicates that they do not have sufficient energy to create GS 118+01−44. Therefore, an additional energy source is needed to explain the genesis of GS 118+01−44. On the other hand, the presence of several H ii regions and young stellar object candidates in the edges of GS 118+01−44 shows that the region is still active in forming new stars.Fil: Suad, Laura Andrea. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Cichowolski, Silvina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Noriega Crespo, A.. Space Telescope Science Institute; Estados UnidosFil: Arnal, Edmundo Marcelo. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Flagey, N.. Space Telescope Science Institute; Estados UnidosEDP Sciences2016-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21538Suad, Laura Andrea; Cichowolski, Silvina; Noriega Crespo, A.; Arnal, Edmundo Marcelo; Testori, Juan Carlos; et al.; The H I supershell GS 118+01-44 and its role in the interstellar medium; EDP Sciences; Astronomy and Astrophysics; 585; A154; 1-2016; 1-110004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201425409info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/01/aa25409-14/aa25409-14.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:53:31Zoai:ri.conicet.gov.ar:11336/21538instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:53:31.511CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| title |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| spellingShingle |
The H I supershell GS 118+01-44 and its role in the interstellar medium Suad, Laura Andrea ISM: bubbles ISM: kinematics and dynamics HII regions stars: formation |
| title_short |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| title_full |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| title_fullStr |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| title_full_unstemmed |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| title_sort |
The H I supershell GS 118+01-44 and its role in the interstellar medium |
| dc.creator.none.fl_str_mv |
Suad, Laura Andrea Cichowolski, Silvina Noriega Crespo, A. Arnal, Edmundo Marcelo Testori, Juan Carlos Flagey, N. |
| author |
Suad, Laura Andrea |
| author_facet |
Suad, Laura Andrea Cichowolski, Silvina Noriega Crespo, A. Arnal, Edmundo Marcelo Testori, Juan Carlos Flagey, N. |
| author_role |
author |
| author2 |
Cichowolski, Silvina Noriega Crespo, A. Arnal, Edmundo Marcelo Testori, Juan Carlos Flagey, N. |
| author2_role |
author author author author author |
| dc.subject.none.fl_str_mv |
ISM: bubbles ISM: kinematics and dynamics HII regions stars: formation |
| topic |
ISM: bubbles ISM: kinematics and dynamics HII regions stars: formation |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Aims. We carry out a multiwavelength study to characterize the H i supershell designated GS 118+01−44, and to analyse its possible origin. Methods. A multiwavelength study has been carried out to study the supershell and its environs. We performed an analysis of the H i, CO, radio continuum, and infrared emission distributions. Results. The Canadian Galactic Plane Survey (CGPS) H i data reveals that GS 118+01−44 is centred at (l,b) = (117°̣7, 1°̣4) with a systemic velocity of −44.3 km s-1. According to Galactic rotation models this structure is located at 3.0 ± 0.6 kpc from the Sun. There are several H ii regions and three supernova remnants (SNRs) catalogued in the region. On the other hand, the analysis of the temperature spectral index distribution shows that in the region there is a predominance of non-thermal emission. Infrared emission shows that cool temperatures dominate the area of the supershell. Concerning the origin of the structure, we found that even though several OB stars belonging to Cas OB5 are located in the interior of GS 118+01−44, an analysis of the energy injected by these stars through their stellar winds indicates that they do not have sufficient energy to create GS 118+01−44. Therefore, an additional energy source is needed to explain the genesis of GS 118+01−44. On the other hand, the presence of several H ii regions and young stellar object candidates in the edges of GS 118+01−44 shows that the region is still active in forming new stars. Fil: Suad, Laura Andrea. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina Fil: Cichowolski, Silvina. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Noriega Crespo, A.. Space Telescope Science Institute; Estados Unidos Fil: Arnal, Edmundo Marcelo. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina Fil: Testori, Juan Carlos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina Fil: Flagey, N.. Space Telescope Science Institute; Estados Unidos |
| description |
Aims. We carry out a multiwavelength study to characterize the H i supershell designated GS 118+01−44, and to analyse its possible origin. Methods. A multiwavelength study has been carried out to study the supershell and its environs. We performed an analysis of the H i, CO, radio continuum, and infrared emission distributions. Results. The Canadian Galactic Plane Survey (CGPS) H i data reveals that GS 118+01−44 is centred at (l,b) = (117°̣7, 1°̣4) with a systemic velocity of −44.3 km s-1. According to Galactic rotation models this structure is located at 3.0 ± 0.6 kpc from the Sun. There are several H ii regions and three supernova remnants (SNRs) catalogued in the region. On the other hand, the analysis of the temperature spectral index distribution shows that in the region there is a predominance of non-thermal emission. Infrared emission shows that cool temperatures dominate the area of the supershell. Concerning the origin of the structure, we found that even though several OB stars belonging to Cas OB5 are located in the interior of GS 118+01−44, an analysis of the energy injected by these stars through their stellar winds indicates that they do not have sufficient energy to create GS 118+01−44. Therefore, an additional energy source is needed to explain the genesis of GS 118+01−44. On the other hand, the presence of several H ii regions and young stellar object candidates in the edges of GS 118+01−44 shows that the region is still active in forming new stars. |
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2016 |
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2016-01 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/21538 Suad, Laura Andrea; Cichowolski, Silvina; Noriega Crespo, A.; Arnal, Edmundo Marcelo; Testori, Juan Carlos; et al.; The H I supershell GS 118+01-44 and its role in the interstellar medium; EDP Sciences; Astronomy and Astrophysics; 585; A154; 1-2016; 1-11 0004-6361 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/21538 |
| identifier_str_mv |
Suad, Laura Andrea; Cichowolski, Silvina; Noriega Crespo, A.; Arnal, Edmundo Marcelo; Testori, Juan Carlos; et al.; The H I supershell GS 118+01-44 and its role in the interstellar medium; EDP Sciences; Astronomy and Astrophysics; 585; A154; 1-2016; 1-11 0004-6361 CONICET Digital CONICET |
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