Investigation in the region of the open cluster Tr 14

CCD UBVRI imaging photometry was carried out in the area of Tr 14. For the first time, we can have an overall view of the lower main sequence of the cluster. It is fully confirmed the anomalous nature of the extinction law. The distance of Tr 14 is stated in d= 3100 pc while its age, derived by the...

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Autores principales: Vázquez, Rubén Ángel, Baume, Gustavo Luis, Feinstein, Alejandro, Prado, P.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1994
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/159708
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spelling I19-R120-10915-1597082023-11-02T20:02:01Z http://sedici.unlp.edu.ar/handle/10915/159708 Investigation in the region of the open cluster Tr 14 Vázquez, Rubén Ángel Baume, Gustavo Luis Feinstein, Alejandro Prado, P. 1994 2023-11-02T14:18:28Z es Astronomía Galaxia tr 14 CCD UBVRI imaging photometry was carried out in the area of Tr 14. For the first time, we can have an overall view of the lower main sequence of the cluster. It is fully confirmed the anomalous nature of the extinction law. The distance of Tr 14 is stated in d= 3100 pc while its age, derived by the fitting of isochrones is about 1x10⁶ yrs. The HR diagram of the cluster shows some stars placed in locations where usually are found contracting stars. Our estimation indicates that an on-going star formation process is taken place with an age spread of 5x10⁶ yrs. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
tr 14
spellingShingle Astronomía
Galaxia
tr 14
Vázquez, Rubén Ángel
Baume, Gustavo Luis
Feinstein, Alejandro
Prado, P.
Investigation in the region of the open cluster Tr 14
topic_facet Astronomía
Galaxia
tr 14
description CCD UBVRI imaging photometry was carried out in the area of Tr 14. For the first time, we can have an overall view of the lower main sequence of the cluster. It is fully confirmed the anomalous nature of the extinction law. The distance of Tr 14 is stated in d= 3100 pc while its age, derived by the fitting of isochrones is about 1x10⁶ yrs. The HR diagram of the cluster shows some stars placed in locations where usually are found contracting stars. Our estimation indicates that an on-going star formation process is taken place with an age spread of 5x10⁶ yrs.
format Articulo
Comunicacion
author Vázquez, Rubén Ángel
Baume, Gustavo Luis
Feinstein, Alejandro
Prado, P.
author_facet Vázquez, Rubén Ángel
Baume, Gustavo Luis
Feinstein, Alejandro
Prado, P.
author_sort Vázquez, Rubén Ángel
title Investigation in the region of the open cluster Tr 14
title_short Investigation in the region of the open cluster Tr 14
title_full Investigation in the region of the open cluster Tr 14
title_fullStr Investigation in the region of the open cluster Tr 14
title_full_unstemmed Investigation in the region of the open cluster Tr 14
title_sort investigation in the region of the open cluster tr 14
publishDate 1994
url http://sedici.unlp.edu.ar/handle/10915/159708
work_keys_str_mv AT vazquezrubenangel investigationintheregionoftheopenclustertr14
AT baumegustavoluis investigationintheregionoftheopenclustertr14
AT feinsteinalejandro investigationintheregionoftheopenclustertr14
AT pradop investigationintheregionoftheopenclustertr14
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