A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33
- Autores
- Barbá, Rodolfo Héctor; Maíz Apellániz, Jesús; Pérez, Enrique; Rubio, Mónica; Bolatto, Alberto; Fariña, Cecilia; Bosch, Guillermo Luis; Walborn, Nolan Revere
- Año de publicación
- 2009
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the first high-spatial-resolution nearinfrared (NIR) imaging of NGC604, obtained with the NICMOS camera onboard the Hubble Space Telescope (HST). These NICMOS broad-band images reveal new NIR point sources, clusters, and diffuse structures. We find an excellent spatial correlation between the 8.4 GHz radio continuum and the 2.2 µm nebular emission. Moreover, massive young stellar object candidates appear aligned with these radio peaks, reinforcing the idea that those areas are star-forming regions. Three different scaled OB associations are recognized in the NICMOS images. The brightest NIR sources in our images have properties that suggest that they are red supergiant stars, of which one was previously known. This preliminary analysis of the NICMOS images shows the complexity of the stellar content of the NGC604 nebula.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Astronomía
Galaxies: starburst
HII regions
ISM: individual (NGC604)
Messier 33
Stars: red supergiants
Stars: early-type
Stars: formation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/93909
Ver los metadatos del registro completo
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A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33Barbá, Rodolfo HéctorMaíz Apellániz, JesúsPérez, EnriqueRubio, MónicaBolatto, AlbertoFariña, CeciliaBosch, Guillermo LuisWalborn, Nolan RevereAstronomíaGalaxies: starburstHII regionsISM: individual (NGC604)Messier 33Stars: red supergiantsStars: early-typeStars: formationWe present the first high-spatial-resolution nearinfrared (NIR) imaging of NGC604, obtained with the NICMOS camera onboard the <i>Hubble Space Telescope</i> (HST). These NICMOS broad-band images reveal new NIR point sources, clusters, and diffuse structures. We find an excellent spatial correlation between the 8.4 GHz radio continuum and the 2.2 µm nebular emission. Moreover, massive young stellar object candidates appear aligned with these radio peaks, reinforcing the idea that those areas are star-forming regions. Three different scaled OB associations are recognized in the NICMOS images. The brightest NIR sources in our images have properties that suggest that they are red supergiant stars, of which one was previously known. This preliminary analysis of the NICMOS images shows the complexity of the stellar content of the NGC604 nebula.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2009-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf309-313http://sedici.unlp.edu.ar/handle/10915/93909enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/handle/11336/44104info:eu-repo/semantics/altIdentifier/issn/0004-640Xinfo:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-009-0104-9info:eu-repo/semantics/altIdentifier/hdl/11336/44104info: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:UNLP2025-09-29T11:19:26Zoai:sedici.unlp.edu.ar:10915/93909Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:19:27.083SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
title |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
spellingShingle |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 Barbá, Rodolfo Héctor Astronomía Galaxies: starburst HII regions ISM: individual (NGC604) Messier 33 Stars: red supergiants Stars: early-type Stars: formation |
title_short |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
title_full |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
title_fullStr |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
title_full_unstemmed |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
title_sort |
A Hubble Space Telescope/NICMOS view of the prototypical giant HII region NGC604 in M33 |
dc.creator.none.fl_str_mv |
Barbá, Rodolfo Héctor Maíz Apellániz, Jesús Pérez, Enrique Rubio, Mónica Bolatto, Alberto Fariña, Cecilia Bosch, Guillermo Luis Walborn, Nolan Revere |
author |
Barbá, Rodolfo Héctor |
author_facet |
Barbá, Rodolfo Héctor Maíz Apellániz, Jesús Pérez, Enrique Rubio, Mónica Bolatto, Alberto Fariña, Cecilia Bosch, Guillermo Luis Walborn, Nolan Revere |
author_role |
author |
author2 |
Maíz Apellániz, Jesús Pérez, Enrique Rubio, Mónica Bolatto, Alberto Fariña, Cecilia Bosch, Guillermo Luis Walborn, Nolan Revere |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
Astronomía Galaxies: starburst HII regions ISM: individual (NGC604) Messier 33 Stars: red supergiants Stars: early-type Stars: formation |
topic |
Astronomía Galaxies: starburst HII regions ISM: individual (NGC604) Messier 33 Stars: red supergiants Stars: early-type Stars: formation |
dc.description.none.fl_txt_mv |
We present the first high-spatial-resolution nearinfrared (NIR) imaging of NGC604, obtained with the NICMOS camera onboard the <i>Hubble Space Telescope</i> (HST). These NICMOS broad-band images reveal new NIR point sources, clusters, and diffuse structures. We find an excellent spatial correlation between the 8.4 GHz radio continuum and the 2.2 µm nebular emission. Moreover, massive young stellar object candidates appear aligned with these radio peaks, reinforcing the idea that those areas are star-forming regions. Three different scaled OB associations are recognized in the NICMOS images. The brightest NIR sources in our images have properties that suggest that they are red supergiant stars, of which one was previously known. This preliminary analysis of the NICMOS images shows the complexity of the stellar content of the NGC604 nebula. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
description |
We present the first high-spatial-resolution nearinfrared (NIR) imaging of NGC604, obtained with the NICMOS camera onboard the <i>Hubble Space Telescope</i> (HST). These NICMOS broad-band images reveal new NIR point sources, clusters, and diffuse structures. We find an excellent spatial correlation between the 8.4 GHz radio continuum and the 2.2 µm nebular emission. Moreover, massive young stellar object candidates appear aligned with these radio peaks, reinforcing the idea that those areas are star-forming regions. Three different scaled OB associations are recognized in the NICMOS images. The brightest NIR sources in our images have properties that suggest that they are red supergiant stars, of which one was previously known. This preliminary analysis of the NICMOS images shows the complexity of the stellar content of the NGC604 nebula. |
publishDate |
2009 |
dc.date.none.fl_str_mv |
2009-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/93909 |
url |
http://sedici.unlp.edu.ar/handle/10915/93909 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/handle/11336/44104 info:eu-repo/semantics/altIdentifier/issn/0004-640X info:eu-repo/semantics/altIdentifier/doi/10.1007/s10509-009-0104-9 info:eu-repo/semantics/altIdentifier/hdl/11336/44104 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 309-313 |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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