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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Formato: | Articulo Comunicacion |
Lenguaje: | Español |
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1994
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/159708 |
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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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1807221730835431424 |