Molecular gas in the star-forming region IRAS 08589-4714
- Autores
- Saldaño, Hugo P.; Vasquez, Javier; Cappa, Cristina Elisabet; Gómez, M.; Duronea, Nicolás Urbano; Rubio, Mónica
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Aims. We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. Methods. We observed the 12CO(3-2), 13CO(3-2), C18O(3-2), HCO+(3-2), and HCN(3-2) molecular lines in a region of 150″ × 150″, centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. Results. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H2 volume density are 310 M⊙ and 1.2 × 104 cm-3, respectively. Two overdensities were identified within the clump in HCN(3-2) and HCO+(3-2) lines. A comparison of the LTE and virial masses suggests that the clump is collapsing in regions that harbor young stellar objects. An analysis of the molecular lines suggests that they are driving molecular outflows.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Circumstellar matter
ISM: individual objects: IRAS 08589-4714
ISM: jets and outflows
ISM: molecules
Stars: formation
Stars: massive - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/85788
Ver los metadatos del registro completo
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Molecular gas in the star-forming region IRAS 08589-4714Saldaño, Hugo P.Vasquez, JavierCappa, Cristina ElisabetGómez, M.Duronea, Nicolás UrbanoRubio, MónicaCiencias AstronómicasCircumstellar matterISM: individual objects: IRAS 08589-4714ISM: jets and outflowsISM: moleculesStars: formationStars: massiveAims. We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. Methods. We observed the <SUP>12</SUP>CO(3-2), <SUP>13</SUP>CO(3-2), C<SUP>18</SUP>O(3-2), HCO<SUP>+</SUP>(3-2), and HCN(3-2) molecular lines in a region of 150″ × 150″, centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. Results. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H<SUB>2</SUB> volume density are 310 M⊙ and 1.2 × 10<SUP>4</SUP> cm<SUP>-3</SUP>, respectively. Two overdensities were identified within the clump in HCN(3-2) and HCO<SUP>+</SUP>(3-2) lines. A comparison of the LTE and virial masses suggests that the clump is collapsing in regions that harbor young stellar objects. An analysis of the molecular lines suggests that they are driving molecular outflows.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2016info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/85788enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201527911info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:57:33Zoai:sedici.unlp.edu.ar:10915/85788Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:57:33.421SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Molecular gas in the star-forming region IRAS 08589-4714 |
| title |
Molecular gas in the star-forming region IRAS 08589-4714 |
| spellingShingle |
Molecular gas in the star-forming region IRAS 08589-4714 Saldaño, Hugo P. Ciencias Astronómicas Circumstellar matter ISM: individual objects: IRAS 08589-4714 ISM: jets and outflows ISM: molecules Stars: formation Stars: massive |
| title_short |
Molecular gas in the star-forming region IRAS 08589-4714 |
| title_full |
Molecular gas in the star-forming region IRAS 08589-4714 |
| title_fullStr |
Molecular gas in the star-forming region IRAS 08589-4714 |
| title_full_unstemmed |
Molecular gas in the star-forming region IRAS 08589-4714 |
| title_sort |
Molecular gas in the star-forming region IRAS 08589-4714 |
| dc.creator.none.fl_str_mv |
Saldaño, Hugo P. Vasquez, Javier Cappa, Cristina Elisabet Gómez, M. Duronea, Nicolás Urbano Rubio, Mónica |
| author |
Saldaño, Hugo P. |
| author_facet |
Saldaño, Hugo P. Vasquez, Javier Cappa, Cristina Elisabet Gómez, M. Duronea, Nicolás Urbano Rubio, Mónica |
| author_role |
author |
| author2 |
Vasquez, Javier Cappa, Cristina Elisabet Gómez, M. Duronea, Nicolás Urbano Rubio, Mónica |
| author2_role |
author author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Circumstellar matter ISM: individual objects: IRAS 08589-4714 ISM: jets and outflows ISM: molecules Stars: formation Stars: massive |
| topic |
Ciencias Astronómicas Circumstellar matter ISM: individual objects: IRAS 08589-4714 ISM: jets and outflows ISM: molecules Stars: formation Stars: massive |
| dc.description.none.fl_txt_mv |
Aims. We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. Methods. We observed the <SUP>12</SUP>CO(3-2), <SUP>13</SUP>CO(3-2), C<SUP>18</SUP>O(3-2), HCO<SUP>+</SUP>(3-2), and HCN(3-2) molecular lines in a region of 150″ × 150″, centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. Results. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H<SUB>2</SUB> volume density are 310 M⊙ and 1.2 × 10<SUP>4</SUP> cm<SUP>-3</SUP>, respectively. Two overdensities were identified within the clump in HCN(3-2) and HCO<SUP>+</SUP>(3-2) lines. A comparison of the LTE and virial masses suggests that the clump is collapsing in regions that harbor young stellar objects. An analysis of the molecular lines suggests that they are driving molecular outflows. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
| description |
Aims. We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. Methods. We observed the <SUP>12</SUP>CO(3-2), <SUP>13</SUP>CO(3-2), C<SUP>18</SUP>O(3-2), HCO<SUP>+</SUP>(3-2), and HCN(3-2) molecular lines in a region of 150″ × 150″, centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. Results. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H<SUB>2</SUB> volume density are 310 M⊙ and 1.2 × 10<SUP>4</SUP> cm<SUP>-3</SUP>, respectively. Two overdensities were identified within the clump in HCN(3-2) and HCO<SUP>+</SUP>(3-2) lines. A comparison of the LTE and virial masses suggests that the clump is collapsing in regions that harbor young stellar objects. An analysis of the molecular lines suggests that they are driving molecular outflows. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016 |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/85788 |
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eng |
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eng |
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