A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122
- Autores
- Duronea, Nicolas Urbano
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Using NANTEN 12CO (J=1-0) observations (HPBW = 2´.7), we found a molecular cloud associated with the star forming regions RCW 121 and RCW 122. Kinematical properties, large scale distribution, and physical parameters were determined. Both RCW 121 and RCW 122, have very strong IR counterparts. New radiocontinuum flux determinations indicate that RCW 121 and RCW 122 are thermal in nature.
Fil: Duronea, Nicolas Urbano. 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
Massive stars: fundamental parameters and circumstellar interactions
Cariló
Argentina
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
ISM: HII regions
ISM: individual objects: RCW 121 and RCW 122 - 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:11336/146155
Ver los metadatos del registro completo
id |
CONICETDig_689d6ec8f08e47957c20f5bdd0beb4b5 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/146155 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122Duronea, Nicolas UrbanoISM: HII regionsISM: individual objects: RCW 121 and RCW 122https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using NANTEN 12CO (J=1-0) observations (HPBW = 2´.7), we found a molecular cloud associated with the star forming regions RCW 121 and RCW 122. Kinematical properties, large scale distribution, and physical parameters were determined. Both RCW 121 and RCW 122, have very strong IR counterparts. New radiocontinuum flux determinations indicate that RCW 121 and RCW 122 are thermal in nature.Fil: Duronea, Nicolas Urbano. 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; ArgentinaMassive stars: fundamental parameters and circumstellar interactionsCarilóArgentinaFacultad de Ciencias Astronómicas y GeofísicasUniversidad Nacional Autónoma de MéxicoBenaglia, PaulaBosch, Guillermo LuisCappa, Cristina Elisabeth2008info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectWorkshopJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/146155A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122; Massive stars: fundamental parameters and circumstellar interactions; Cariló; Argentina; 2006; 161-1611405-2059CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol33.htmlinfo:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_nduronea.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:17:34Zoai:ri.conicet.gov.ar:11336/146155instacron: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 10:17:34.754CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
title |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
spellingShingle |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 Duronea, Nicolas Urbano ISM: HII regions ISM: individual objects: RCW 121 and RCW 122 |
title_short |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
title_full |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
title_fullStr |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
title_full_unstemmed |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
title_sort |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122 |
dc.creator.none.fl_str_mv |
Duronea, Nicolas Urbano |
author |
Duronea, Nicolas Urbano |
author_facet |
Duronea, Nicolas Urbano |
author_role |
author |
dc.contributor.none.fl_str_mv |
Benaglia, Paula Bosch, Guillermo Luis Cappa, Cristina Elisabeth |
dc.subject.none.fl_str_mv |
ISM: HII regions ISM: individual objects: RCW 121 and RCW 122 |
topic |
ISM: HII regions ISM: individual objects: RCW 121 and RCW 122 |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Using NANTEN 12CO (J=1-0) observations (HPBW = 2´.7), we found a molecular cloud associated with the star forming regions RCW 121 and RCW 122. Kinematical properties, large scale distribution, and physical parameters were determined. Both RCW 121 and RCW 122, have very strong IR counterparts. New radiocontinuum flux determinations indicate that RCW 121 and RCW 122 are thermal in nature. Fil: Duronea, Nicolas Urbano. 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 Massive stars: fundamental parameters and circumstellar interactions Cariló Argentina Facultad de Ciencias Astronómicas y Geofísicas |
description |
Using NANTEN 12CO (J=1-0) observations (HPBW = 2´.7), we found a molecular cloud associated with the star forming regions RCW 121 and RCW 122. Kinematical properties, large scale distribution, and physical parameters were determined. Both RCW 121 and RCW 122, have very strong IR counterparts. New radiocontinuum flux determinations indicate that RCW 121 and RCW 122 are thermal in nature. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Workshop Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
status_str |
publishedVersion |
format |
conferenceObject |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/146155 A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122; Massive stars: fundamental parameters and circumstellar interactions; Cariló; Argentina; 2006; 161-161 1405-2059 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/146155 |
identifier_str_mv |
A 12CO (J=1-0) study towards the star forming regions RCW 121 and RCW 122; Massive stars: fundamental parameters and circumstellar interactions; Cariló; Argentina; 2006; 161-161 1405-2059 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol33.html info:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..33/PDF/RMxAC..33_nduronea.pdf |
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 application/pdf |
dc.coverage.none.fl_str_mv |
Internacional |
dc.publisher.none.fl_str_mv |
Universidad Nacional Autónoma de México |
publisher.none.fl_str_mv |
Universidad Nacional Autónoma de México |
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 |
_version_ |
1844614129878302720 |
score |
13.070432 |