G287.84-0.82: an infrared star cluster in the Carina nebula

We have studied the properties of an infrared cluster embedded in the gas and dust of the southern part of the Carina nebula (NGC 3372), where the probable existence of current star formation has already been predicted. We used mid-infrared (A and C bands) and near-infrared (JHK<SUB>s</SUB&...

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Autores principales: Hägele, Guillermo Federico, Albacete Colombo, Juan Facundo, Barbá, Rodolfo Héctor, Bosch, Guillermo Luis
Formato: Articulo
Lenguaje:Inglés
Publicado: 2004
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83280
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id I19-R120-10915-83280
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Infrared: stars
Open clusters and associations: individual: carina nebula
Open clusters and associations: individual: G287.84-0.82
Open clusters and associations: individual: NGC 3372
Stars: formation
Stars: pre-main-sequence
spellingShingle Ciencias Astronómicas
Infrared: stars
Open clusters and associations: individual: carina nebula
Open clusters and associations: individual: G287.84-0.82
Open clusters and associations: individual: NGC 3372
Stars: formation
Stars: pre-main-sequence
Hägele, Guillermo Federico
Albacete Colombo, Juan Facundo
Barbá, Rodolfo Héctor
Bosch, Guillermo Luis
G287.84-0.82: an infrared star cluster in the Carina nebula
topic_facet Ciencias Astronómicas
Infrared: stars
Open clusters and associations: individual: carina nebula
Open clusters and associations: individual: G287.84-0.82
Open clusters and associations: individual: NGC 3372
Stars: formation
Stars: pre-main-sequence
description We have studied the properties of an infrared cluster embedded in the gas and dust of the southern part of the Carina nebula (NGC 3372), where the probable existence of current star formation has already been predicted. We used mid-infrared (A and C bands) and near-infrared (JHK<SUB>s</SUB>) images from the Midcourse Space Experiment and the Two-Micron All-Sky Survey, respectively, combined with an optical Ha narrow-band filter image obtained at the Cerro Tololo Inter-American Observatory. The infrared star cluster has at least 17 members, and its parameters, radius and stellar density are in very good agreement with high- to intermediate-mass star formation scenarios. The detected infrared sources have roughly the same intrinsic infrared excess determined from their position in colour-colour and colour-magnitude diagrams, suggesting that these objects could be related to pre-main-sequence stars of high to intermediate mass. Furthermore, we present a low-dispersion spectrum of the LS 1883 (O9.5V) star located near the centre of the infrared cluster. The position of this object in the colour-colour and colour-magnitude infrared diagrams lies close to the reddening vector of a zero-age main-sequence O9V spectral-type star, and it seems to be the first star of this cluster to emerge. All these facts are consistent with the current star-forming scenarios associated with highly embedded star clusters.
format Articulo
Articulo
author Hägele, Guillermo Federico
Albacete Colombo, Juan Facundo
Barbá, Rodolfo Héctor
Bosch, Guillermo Luis
author_facet Hägele, Guillermo Federico
Albacete Colombo, Juan Facundo
Barbá, Rodolfo Héctor
Bosch, Guillermo Luis
author_sort Hägele, Guillermo Federico
title G287.84-0.82: an infrared star cluster in the Carina nebula
title_short G287.84-0.82: an infrared star cluster in the Carina nebula
title_full G287.84-0.82: an infrared star cluster in the Carina nebula
title_fullStr G287.84-0.82: an infrared star cluster in the Carina nebula
title_full_unstemmed G287.84-0.82: an infrared star cluster in the Carina nebula
title_sort g287.84-0.82: an infrared star cluster in the carina nebula
publishDate 2004
url http://sedici.unlp.edu.ar/handle/10915/83280
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AT albacetecolombojuanfacundo g28784082aninfraredstarclusterinthecarinanebula
AT barbarodolfohector g28784082aninfraredstarclusterinthecarinanebula
AT boschguillermoluis g28784082aninfraredstarclusterinthecarinanebula
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