Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula
- Autores
- Brandner, Wolfgang; Grebel, Eva K.; Barba, Rodolfo Héctor; Walborn, Nolan Revere; Moneti, Andrea
- Año de publicación
- 2001
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present the detection of an intermediate-mass, pre-main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST/ NICMOS. In addition to four previously known luminous Class I infrared "protostars," the NICMOS data reveal 20 new sources with intrinsic infrared excess similar to Galactic pre-main-sequence stars. Based on their infrared brightness, these objects can be identified as the LMC equivalent of Galactic pre-main-sequence stars. The faintest LMC young stellar objects in the sample have colors similar to T Tauri stars and have about the same brightness as T Tauri stars if placed at the distance of the LMC. We find no evidence for a lower mass cutoff in the initial mass function. Instead, the whole spectrum of stellar masses from pre-main-sequence stars with ∼1.5 M⊙ to massive O stars still embedded in dense knots appears to be present in the nebular filaments. The majority of the young stellar objects can be found to the north of the central starburst cluster R136. This region is very likely evolving into an OB association. The observations provide further evidence that star formation in the 30 Doradus region is very similar to Galactic star formation and confirm the presence of sequential star formation in 30 Doradus, with present-day star formation taking place in the arc of molecular gas to the north and west of the starburst cluster.
Fil: Brandner, Wolfgang. European Southern Observatory; Alemania. University of Hawaii at Manoa; Estados Unidos
Fil: Grebel, Eva K.. Max-Planck-Institut Astronomie; Alemania
Fil: Barba, Rodolfo Héctor. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina
Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos
Fil: Moneti, Andrea. Institut D’astrophysique de Paris; Francia - Materia
-
GALAXIES: STELLAR CONTENT
MAGELLANIC CLOUDS
STARS: FORMATION
STARS: PRE-MAIN-SEQUENCE - 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:11336/214200
Ver los metadatos del registro completo
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Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebulaBrandner, WolfgangGrebel, Eva K.Barba, Rodolfo HéctorWalborn, Nolan RevereMoneti, AndreaGALAXIES: STELLAR CONTENTMAGELLANIC CLOUDSSTARS: FORMATIONSTARS: PRE-MAIN-SEQUENCEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the detection of an intermediate-mass, pre-main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST/ NICMOS. In addition to four previously known luminous Class I infrared "protostars," the NICMOS data reveal 20 new sources with intrinsic infrared excess similar to Galactic pre-main-sequence stars. Based on their infrared brightness, these objects can be identified as the LMC equivalent of Galactic pre-main-sequence stars. The faintest LMC young stellar objects in the sample have colors similar to T Tauri stars and have about the same brightness as T Tauri stars if placed at the distance of the LMC. We find no evidence for a lower mass cutoff in the initial mass function. Instead, the whole spectrum of stellar masses from pre-main-sequence stars with ∼1.5 M⊙ to massive O stars still embedded in dense knots appears to be present in the nebular filaments. The majority of the young stellar objects can be found to the north of the central starburst cluster R136. This region is very likely evolving into an OB association. The observations provide further evidence that star formation in the 30 Doradus region is very similar to Galactic star formation and confirm the presence of sequential star formation in 30 Doradus, with present-day star formation taking place in the arc of molecular gas to the north and west of the starburst cluster.Fil: Brandner, Wolfgang. European Southern Observatory; Alemania. University of Hawaii at Manoa; Estados UnidosFil: Grebel, Eva K.. Max-Planck-Institut Astronomie; AlemaniaFil: Barba, Rodolfo Héctor. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; ArgentinaFil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados UnidosFil: Moneti, Andrea. Institut D’astrophysique de Paris; FranciaIOP Publishing2001-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/214200Brandner, Wolfgang; Grebel, Eva K.; Barba, Rodolfo Héctor; Walborn, Nolan Revere; Moneti, Andrea; Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula; IOP Publishing; Astronomical Journal; 122; 2; 12-2001; 858-8650004-6256CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/322065info:eu-repo/semantics/altIdentifier/doi/10.1086/322065info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:19:27Zoai:ri.conicet.gov.ar:11336/214200instacron: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 10:19:28.25CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
title |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
spellingShingle |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula Brandner, Wolfgang GALAXIES: STELLAR CONTENT MAGELLANIC CLOUDS STARS: FORMATION STARS: PRE-MAIN-SEQUENCE |
title_short |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
title_full |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
title_fullStr |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
title_full_unstemmed |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
title_sort |
Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula |
dc.creator.none.fl_str_mv |
Brandner, Wolfgang Grebel, Eva K. Barba, Rodolfo Héctor Walborn, Nolan Revere Moneti, Andrea |
author |
Brandner, Wolfgang |
author_facet |
Brandner, Wolfgang Grebel, Eva K. Barba, Rodolfo Héctor Walborn, Nolan Revere Moneti, Andrea |
author_role |
author |
author2 |
Grebel, Eva K. Barba, Rodolfo Héctor Walborn, Nolan Revere Moneti, Andrea |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
GALAXIES: STELLAR CONTENT MAGELLANIC CLOUDS STARS: FORMATION STARS: PRE-MAIN-SEQUENCE |
topic |
GALAXIES: STELLAR CONTENT MAGELLANIC CLOUDS STARS: FORMATION STARS: PRE-MAIN-SEQUENCE |
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 present the detection of an intermediate-mass, pre-main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST/ NICMOS. In addition to four previously known luminous Class I infrared "protostars," the NICMOS data reveal 20 new sources with intrinsic infrared excess similar to Galactic pre-main-sequence stars. Based on their infrared brightness, these objects can be identified as the LMC equivalent of Galactic pre-main-sequence stars. The faintest LMC young stellar objects in the sample have colors similar to T Tauri stars and have about the same brightness as T Tauri stars if placed at the distance of the LMC. We find no evidence for a lower mass cutoff in the initial mass function. Instead, the whole spectrum of stellar masses from pre-main-sequence stars with ∼1.5 M⊙ to massive O stars still embedded in dense knots appears to be present in the nebular filaments. The majority of the young stellar objects can be found to the north of the central starburst cluster R136. This region is very likely evolving into an OB association. The observations provide further evidence that star formation in the 30 Doradus region is very similar to Galactic star formation and confirm the presence of sequential star formation in 30 Doradus, with present-day star formation taking place in the arc of molecular gas to the north and west of the starburst cluster. Fil: Brandner, Wolfgang. European Southern Observatory; Alemania. University of Hawaii at Manoa; Estados Unidos Fil: Grebel, Eva K.. Max-Planck-Institut Astronomie; Alemania Fil: Barba, Rodolfo Héctor. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio. Universidad Nacional de San Juan. Instituto de Ciencias Astronómicas, de la Tierra y del Espacio; Argentina Fil: Walborn, Nolan Revere. Space Telescope Science Institute; Estados Unidos Fil: Moneti, Andrea. Institut D’astrophysique de Paris; Francia |
description |
We present the detection of an intermediate-mass, pre-main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST/ NICMOS. In addition to four previously known luminous Class I infrared "protostars," the NICMOS data reveal 20 new sources with intrinsic infrared excess similar to Galactic pre-main-sequence stars. Based on their infrared brightness, these objects can be identified as the LMC equivalent of Galactic pre-main-sequence stars. The faintest LMC young stellar objects in the sample have colors similar to T Tauri stars and have about the same brightness as T Tauri stars if placed at the distance of the LMC. We find no evidence for a lower mass cutoff in the initial mass function. Instead, the whole spectrum of stellar masses from pre-main-sequence stars with ∼1.5 M⊙ to massive O stars still embedded in dense knots appears to be present in the nebular filaments. The majority of the young stellar objects can be found to the north of the central starburst cluster R136. This region is very likely evolving into an OB association. The observations provide further evidence that star formation in the 30 Doradus region is very similar to Galactic star formation and confirm the presence of sequential star formation in 30 Doradus, with present-day star formation taking place in the arc of molecular gas to the north and west of the starburst cluster. |
publishDate |
2001 |
dc.date.none.fl_str_mv |
2001-12 |
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/11336/214200 Brandner, Wolfgang; Grebel, Eva K.; Barba, Rodolfo Héctor; Walborn, Nolan Revere; Moneti, Andrea; Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula; IOP Publishing; Astronomical Journal; 122; 2; 12-2001; 858-865 0004-6256 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/214200 |
identifier_str_mv |
Brandner, Wolfgang; Grebel, Eva K.; Barba, Rodolfo Héctor; Walborn, Nolan Revere; Moneti, Andrea; Hubble space telescope nicmos detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 doradus nebula; IOP Publishing; Astronomical Journal; 122; 2; 12-2001; 858-865 0004-6256 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://iopscience.iop.org/article/10.1086/322065 info:eu-repo/semantics/altIdentifier/doi/10.1086/322065 |
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 |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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1844614166514499584 |
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13.070432 |