HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52
- Autores
- Cappa, Cristina Elisabeth; Niemela, Virpi S.; Martin, Maria Cristina; McClure Griffiths, Naomi M.
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We analyze the interstellar medium in the environs of two hot and massive stars, HD 92809 (= WR 23, WC6) and LSS 1887 (O8V), which ionize the optical ring nebulae Anon(WR 23) and RCW 52, respectively. Our analysis is based on neutral hydrogen (Hi) 21cm line data, which reveal interstellar bubbles surrounding the massive stars and their optical ring nebulae. The Hi bubble related to WR 23 is 13.3 pc in radius and is expanding at 10 km s −1 . The associated atomic neutral mass amounts to 830 M . The Hi structure related to LSS 1887 is about 6.3 pc in radius, has an expansion velocity of 7 km s −1 and an associated atomic neutral mass of 100 M . These Hi features are the neutral counterparts of the optical ring nebulae and were mainly created by the action of the stellar winds of the massive stars on their environs. The dynamical age of the Hi bubble around WR 23 (7×105 yr) suggests that it was created during the WR phase of stellar evolution. However, the large tangential motions of WR 23 and LSS 1887 suggest that part of the observed optical and Hi structures may be due to a bow shock. The analysis of the distribution of emission in the far infrared and in the CO(1-0) molecular line in the environs of WR 23 and LSS 1887, reveals that there are also infrared and molecular counterparts of the detected Hi bubbles.
Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Niemela, Virpi S.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Martin, Maria Cristina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: McClure Griffiths, Naomi M.. Australia Telescope National Facility; Australia - Materia
-
Interstellar bubbles
HII regions
Ring nebulae
Anon (WR 23)
RCW52 (estrella)
Early-type stars
Wolf-Rayet stars
WR 23 (estrella)
LSS 1887 (estrella) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/29551
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/29551 |
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3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52Cappa, Cristina ElisabethNiemela, Virpi S.Martin, Maria CristinaMcClure Griffiths, Naomi M.Interstellar bubblesHII regionsRing nebulaeAnon (WR 23)RCW52 (estrella)Early-type starsWolf-Rayet starsWR 23 (estrella)LSS 1887 (estrella)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We analyze the interstellar medium in the environs of two hot and massive stars, HD 92809 (= WR 23, WC6) and LSS 1887 (O8V), which ionize the optical ring nebulae Anon(WR 23) and RCW 52, respectively. Our analysis is based on neutral hydrogen (Hi) 21cm line data, which reveal interstellar bubbles surrounding the massive stars and their optical ring nebulae. The Hi bubble related to WR 23 is 13.3 pc in radius and is expanding at 10 km s −1 . The associated atomic neutral mass amounts to 830 M . The Hi structure related to LSS 1887 is about 6.3 pc in radius, has an expansion velocity of 7 km s −1 and an associated atomic neutral mass of 100 M . These Hi features are the neutral counterparts of the optical ring nebulae and were mainly created by the action of the stellar winds of the massive stars on their environs. The dynamical age of the Hi bubble around WR 23 (7×105 yr) suggests that it was created during the WR phase of stellar evolution. However, the large tangential motions of WR 23 and LSS 1887 suggest that part of the observed optical and Hi structures may be due to a bow shock. The analysis of the distribution of emission in the far infrared and in the CO(1-0) molecular line in the environs of WR 23 and LSS 1887, reveals that there are also infrared and molecular counterparts of the detected Hi bubbles.Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Niemela, Virpi S.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Martin, Maria Cristina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: McClure Griffiths, Naomi M.. Australia Telescope National Facility; AustraliaEDP Sciences2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/29551Cappa, Cristina Elisabeth; Niemela, Virpi S.; Martin, Maria Cristina; McClure Griffiths, Naomi M.; HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52; EDP Sciences; Astronomy and Astrophysics; 436; 12-2005; 155-1630004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20042344info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2005/22/aa2344-04/aa2344-04.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 Técnicas2025-09-29T10:46:13Zoai:ri.conicet.gov.ar:11336/29551instacron: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 10:46:13.331CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
title |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
spellingShingle |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 Cappa, Cristina Elisabeth Interstellar bubbles HII regions Ring nebulae Anon (WR 23) RCW52 (estrella) Early-type stars Wolf-Rayet stars WR 23 (estrella) LSS 1887 (estrella) |
title_short |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
title_full |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
title_fullStr |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
title_full_unstemmed |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
title_sort |
HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52 |
dc.creator.none.fl_str_mv |
Cappa, Cristina Elisabeth Niemela, Virpi S. Martin, Maria Cristina McClure Griffiths, Naomi M. |
author |
Cappa, Cristina Elisabeth |
author_facet |
Cappa, Cristina Elisabeth Niemela, Virpi S. Martin, Maria Cristina McClure Griffiths, Naomi M. |
author_role |
author |
author2 |
Niemela, Virpi S. Martin, Maria Cristina McClure Griffiths, Naomi M. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Interstellar bubbles HII regions Ring nebulae Anon (WR 23) RCW52 (estrella) Early-type stars Wolf-Rayet stars WR 23 (estrella) LSS 1887 (estrella) |
topic |
Interstellar bubbles HII regions Ring nebulae Anon (WR 23) RCW52 (estrella) Early-type stars Wolf-Rayet stars WR 23 (estrella) LSS 1887 (estrella) |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We analyze the interstellar medium in the environs of two hot and massive stars, HD 92809 (= WR 23, WC6) and LSS 1887 (O8V), which ionize the optical ring nebulae Anon(WR 23) and RCW 52, respectively. Our analysis is based on neutral hydrogen (Hi) 21cm line data, which reveal interstellar bubbles surrounding the massive stars and their optical ring nebulae. The Hi bubble related to WR 23 is 13.3 pc in radius and is expanding at 10 km s −1 . The associated atomic neutral mass amounts to 830 M . The Hi structure related to LSS 1887 is about 6.3 pc in radius, has an expansion velocity of 7 km s −1 and an associated atomic neutral mass of 100 M . These Hi features are the neutral counterparts of the optical ring nebulae and were mainly created by the action of the stellar winds of the massive stars on their environs. The dynamical age of the Hi bubble around WR 23 (7×105 yr) suggests that it was created during the WR phase of stellar evolution. However, the large tangential motions of WR 23 and LSS 1887 suggest that part of the observed optical and Hi structures may be due to a bow shock. The analysis of the distribution of emission in the far infrared and in the CO(1-0) molecular line in the environs of WR 23 and LSS 1887, reveals that there are also infrared and molecular counterparts of the detected Hi bubbles. Fil: Cappa, Cristina Elisabeth. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Niemela, Virpi S.. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Martin, Maria Cristina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: McClure Griffiths, Naomi M.. Australia Telescope National Facility; Australia |
description |
We analyze the interstellar medium in the environs of two hot and massive stars, HD 92809 (= WR 23, WC6) and LSS 1887 (O8V), which ionize the optical ring nebulae Anon(WR 23) and RCW 52, respectively. Our analysis is based on neutral hydrogen (Hi) 21cm line data, which reveal interstellar bubbles surrounding the massive stars and their optical ring nebulae. The Hi bubble related to WR 23 is 13.3 pc in radius and is expanding at 10 km s −1 . The associated atomic neutral mass amounts to 830 M . The Hi structure related to LSS 1887 is about 6.3 pc in radius, has an expansion velocity of 7 km s −1 and an associated atomic neutral mass of 100 M . These Hi features are the neutral counterparts of the optical ring nebulae and were mainly created by the action of the stellar winds of the massive stars on their environs. The dynamical age of the Hi bubble around WR 23 (7×105 yr) suggests that it was created during the WR phase of stellar evolution. However, the large tangential motions of WR 23 and LSS 1887 suggest that part of the observed optical and Hi structures may be due to a bow shock. The analysis of the distribution of emission in the far infrared and in the CO(1-0) molecular line in the environs of WR 23 and LSS 1887, reveals that there are also infrared and molecular counterparts of the detected Hi bubbles. |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/29551 Cappa, Cristina Elisabeth; Niemela, Virpi S.; Martin, Maria Cristina; McClure Griffiths, Naomi M.; HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52; EDP Sciences; Astronomy and Astrophysics; 436; 12-2005; 155-163 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/29551 |
identifier_str_mv |
Cappa, Cristina Elisabeth; Niemela, Virpi S.; Martin, Maria Cristina; McClure Griffiths, Naomi M.; HI bubbles surrounding southern optical ring nebulae: Anon(WR 23) and RCW 52; EDP Sciences; Astronomy and Astrophysics; 436; 12-2005; 155-163 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20042344 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2005/22/aa2344-04/aa2344-04.html |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614503218544640 |
score |
13.070432 |