A 12CO (J = 1 -> 0) study towards the Ara OB1 region
- Autores
- Arnal, Edmundo Marcelo; May, J.; Romero, Gisela Andrea
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Intermediate angular resolution (HPBW = 8. 0 7) carbon monoxide (12CO J = 1→0) line observations towards the OB association Ara OB1 are reported. The molecular line observations cover an area of 2. ◦75 × 3. ◦00, and disclose a rich and complex distribution of the molecular line emission. The molecular features likely to be associated with the OB-association Ara OB1 span the velocity range from −28 to −20 km s−1. The most negative radial velocities are observed along NGC 6188 (≡Rim nebula). This nebula marks the interface between the H region RCW 108 and the highly absorbing molecular material located westwards of the ionised region. The dominant CO structures, labeled E and F, have a radial velocity of about −23.5 and −21.8 km s−1, respectively. The former harbours a bright optical knot, the infrared cluster RCW-108 and the strong IRAS source 16362−4845. IRAS point sources are also seen in projection onto 12CO concentrations F and H. This may indicate that the star forming process is a widespread phenomenon in this molecular complex. Extended continuum emission, having a high degree of spatial correlation with both the infrared and molecular emission, is observed in the region. We believe that this emission, thermal in nature, arises from the ionised surface layers of the molecular complex. The ionising agents are the high mass stars of NGC 6193, the nucleus of Ara OB1. The total amount of molecular gas related to Ara OB1 is about ∼1.4×104 M .
Fil: Arnal, Edmundo Marcelo. 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. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: May, J.. Universidad de Chile; Chile
Fil: Romero, Gisela Andrea. 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 - Materia
-
HII regions
RCW 108 (región HII)
Interstellar medium
Open clusters
NGC 6193 (galaxia)
Ara OB1
Radio continuum
Radio lines - 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:11336/30787
Ver los metadatos del registro completo
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A 12CO (J = 1 -> 0) study towards the Ara OB1 regionArnal, Edmundo MarceloMay, J.Romero, Gisela AndreaHII regionsRCW 108 (región HII)Interstellar mediumOpen clustersNGC 6193 (galaxia)Ara OB1Radio continuumRadio lineshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Intermediate angular resolution (HPBW = 8. 0 7) carbon monoxide (12CO J = 1→0) line observations towards the OB association Ara OB1 are reported. The molecular line observations cover an area of 2. ◦75 × 3. ◦00, and disclose a rich and complex distribution of the molecular line emission. The molecular features likely to be associated with the OB-association Ara OB1 span the velocity range from −28 to −20 km s−1. The most negative radial velocities are observed along NGC 6188 (≡Rim nebula). This nebula marks the interface between the H region RCW 108 and the highly absorbing molecular material located westwards of the ionised region. The dominant CO structures, labeled E and F, have a radial velocity of about −23.5 and −21.8 km s−1, respectively. The former harbours a bright optical knot, the infrared cluster RCW-108 and the strong IRAS source 16362−4845. IRAS point sources are also seen in projection onto 12CO concentrations F and H. This may indicate that the star forming process is a widespread phenomenon in this molecular complex. Extended continuum emission, having a high degree of spatial correlation with both the infrared and molecular emission, is observed in the region. We believe that this emission, thermal in nature, arises from the ionised surface layers of the molecular complex. The ionising agents are the high mass stars of NGC 6193, the nucleus of Ara OB1. The total amount of molecular gas related to Ara OB1 is about ∼1.4×104 M .Fil: Arnal, Edmundo Marcelo. 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. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: May, J.. Universidad de Chile; ChileFil: Romero, Gisela Andrea. 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; ArgentinaEDP Sciences2003-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/30787Romero, Gisela Andrea; May, J.; Arnal, Edmundo Marcelo; A 12CO (J = 1 -> 0) study towards the Ara OB1 region; EDP Sciences; Astronomy and Astrophysics; 412; 12-2003; 431-4450004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2003A%26A...412..431Ainfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20031455info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2003/48/aah4540/aah4540.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 Técnicas2025-09-29T10:17:43Zoai:ri.conicet.gov.ar:11336/30787instacron: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 10:17:43.333CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
title |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
spellingShingle |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region Arnal, Edmundo Marcelo HII regions RCW 108 (región HII) Interstellar medium Open clusters NGC 6193 (galaxia) Ara OB1 Radio continuum Radio lines |
title_short |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
title_full |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
title_fullStr |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
title_full_unstemmed |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
title_sort |
A 12CO (J = 1 -> 0) study towards the Ara OB1 region |
dc.creator.none.fl_str_mv |
Arnal, Edmundo Marcelo May, J. Romero, Gisela Andrea |
author |
Arnal, Edmundo Marcelo |
author_facet |
Arnal, Edmundo Marcelo May, J. Romero, Gisela Andrea |
author_role |
author |
author2 |
May, J. Romero, Gisela Andrea |
author2_role |
author author |
dc.subject.none.fl_str_mv |
HII regions RCW 108 (región HII) Interstellar medium Open clusters NGC 6193 (galaxia) Ara OB1 Radio continuum Radio lines |
topic |
HII regions RCW 108 (región HII) Interstellar medium Open clusters NGC 6193 (galaxia) Ara OB1 Radio continuum Radio lines |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Intermediate angular resolution (HPBW = 8. 0 7) carbon monoxide (12CO J = 1→0) line observations towards the OB association Ara OB1 are reported. The molecular line observations cover an area of 2. ◦75 × 3. ◦00, and disclose a rich and complex distribution of the molecular line emission. The molecular features likely to be associated with the OB-association Ara OB1 span the velocity range from −28 to −20 km s−1. The most negative radial velocities are observed along NGC 6188 (≡Rim nebula). This nebula marks the interface between the H region RCW 108 and the highly absorbing molecular material located westwards of the ionised region. The dominant CO structures, labeled E and F, have a radial velocity of about −23.5 and −21.8 km s−1, respectively. The former harbours a bright optical knot, the infrared cluster RCW-108 and the strong IRAS source 16362−4845. IRAS point sources are also seen in projection onto 12CO concentrations F and H. This may indicate that the star forming process is a widespread phenomenon in this molecular complex. Extended continuum emission, having a high degree of spatial correlation with both the infrared and molecular emission, is observed in the region. We believe that this emission, thermal in nature, arises from the ionised surface layers of the molecular complex. The ionising agents are the high mass stars of NGC 6193, the nucleus of Ara OB1. The total amount of molecular gas related to Ara OB1 is about ∼1.4×104 M . Fil: Arnal, Edmundo Marcelo. 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. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: May, J.. Universidad de Chile; Chile Fil: Romero, Gisela Andrea. 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 |
description |
Intermediate angular resolution (HPBW = 8. 0 7) carbon monoxide (12CO J = 1→0) line observations towards the OB association Ara OB1 are reported. The molecular line observations cover an area of 2. ◦75 × 3. ◦00, and disclose a rich and complex distribution of the molecular line emission. The molecular features likely to be associated with the OB-association Ara OB1 span the velocity range from −28 to −20 km s−1. The most negative radial velocities are observed along NGC 6188 (≡Rim nebula). This nebula marks the interface between the H region RCW 108 and the highly absorbing molecular material located westwards of the ionised region. The dominant CO structures, labeled E and F, have a radial velocity of about −23.5 and −21.8 km s−1, respectively. The former harbours a bright optical knot, the infrared cluster RCW-108 and the strong IRAS source 16362−4845. IRAS point sources are also seen in projection onto 12CO concentrations F and H. This may indicate that the star forming process is a widespread phenomenon in this molecular complex. Extended continuum emission, having a high degree of spatial correlation with both the infrared and molecular emission, is observed in the region. We believe that this emission, thermal in nature, arises from the ionised surface layers of the molecular complex. The ionising agents are the high mass stars of NGC 6193, the nucleus of Ara OB1. The total amount of molecular gas related to Ara OB1 is about ∼1.4×104 M . |
publishDate |
2003 |
dc.date.none.fl_str_mv |
2003-12 |
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/11336/30787 Romero, Gisela Andrea; May, J.; Arnal, Edmundo Marcelo; A 12CO (J = 1 -> 0) study towards the Ara OB1 region; EDP Sciences; Astronomy and Astrophysics; 412; 12-2003; 431-445 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/30787 |
identifier_str_mv |
Romero, Gisela Andrea; May, J.; Arnal, Edmundo Marcelo; A 12CO (J = 1 -> 0) study towards the Ara OB1 region; EDP Sciences; Astronomy and Astrophysics; 412; 12-2003; 431-445 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/url/http://adsabs.harvard.edu/abs/2003A%26A...412..431A info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20031455 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2003/48/aah4540/aah4540.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) |
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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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13.070432 |