The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives?
- Autores
- Corti, Mariela Alejandra; Arnal, Edmundo Marcelo
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness temperature minimum in the HI distribution that is surrounded by walls of HI emission. McClure-Griffiths et al. (2002) reported the discovery of GSH263+00+47, centered at (l,b) = (263°.0, 0°.0). The OB association Bochum 7 (l,b) = (265°.0, -2°.0) is seen in projection onto the outer border of GSH263+00+47.
Instituto de Astrofísica de La Plata
Instituto Argentino de Radioastronomía - Materia
-
Astronomía
Física
Ciencias Exactas
HI supershells
Induced star formation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/97312
Ver los metadatos del registro completo
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The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives?Corti, Mariela AlejandraArnal, Edmundo MarceloAstronomíaFísicaCiencias ExactasHI supershellsInduced star formationNeutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness temperature minimum in the HI distribution that is surrounded by walls of HI emission. McClure-Griffiths et al. (2002) reported the discovery of GSH263+00+47, centered at (l,b) = (263°.0, 0°.0). The OB association Bochum 7 (l,b) = (265°.0, -2°.0) is seen in projection onto the outer border of GSH263+00+47.Instituto de Astrofísica de La PlataInstituto Argentino de Radioastronomía2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf160-160http://sedici.unlp.edu.ar/handle/10915/97312enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/82429info:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_mcorti2.pdfinfo:eu-repo/semantics/altIdentifier/issn/0185-1101info:eu-repo/semantics/altIdentifier/hdl/11336/82429info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/2.5/ar/Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:01:16Zoai:sedici.unlp.edu.ar:10915/97312Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:01:16.788SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| title |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| spellingShingle |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? Corti, Mariela Alejandra Astronomía Física Ciencias Exactas HI supershells Induced star formation |
| title_short |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| title_full |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| title_fullStr |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| title_full_unstemmed |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| title_sort |
The new HI supershell GS263-02+45 and the OB Association Bochum 7: close relatives? |
| dc.creator.none.fl_str_mv |
Corti, Mariela Alejandra Arnal, Edmundo Marcelo |
| author |
Corti, Mariela Alejandra |
| author_facet |
Corti, Mariela Alejandra Arnal, Edmundo Marcelo |
| author_role |
author |
| author2 |
Arnal, Edmundo Marcelo |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Astronomía Física Ciencias Exactas HI supershells Induced star formation |
| topic |
Astronomía Física Ciencias Exactas HI supershells Induced star formation |
| dc.description.none.fl_txt_mv |
Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness temperature minimum in the HI distribution that is surrounded by walls of HI emission. McClure-Griffiths et al. (2002) reported the discovery of GSH263+00+47, centered at (l,b) = (263°.0, 0°.0). The OB association Bochum 7 (l,b) = (265°.0, -2°.0) is seen in projection onto the outer border of GSH263+00+47. Instituto de Astrofísica de La Plata Instituto Argentino de Radioastronomía |
| description |
Neutral hydrogen (HI) supershells are usually identified, in a given velocity range, as a brightness temperature minimum in the HI distribution that is surrounded by walls of HI emission. McClure-Griffiths et al. (2002) reported the discovery of GSH263+00+47, centered at (l,b) = (263°.0, 0°.0). The OB association Bochum 7 (l,b) = (265°.0, -2°.0) is seen in projection onto the outer border of GSH263+00+47. |
| publishDate |
2008 |
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2008-12 |
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