Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud

Aims. With the aim of enlarging the number of studied LMC clusters in the age range 8.0 ≈ log(t) ≈ 9.0, we focus here on a sample of mostly unstudied cluster candidates. Methods. We present for the first time CCD Washington CT 1T 2 photometry of stars in the field of 26 LMC clusters. Results. The st...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2012
Materias:
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v540_n_p_Piatti
http://hdl.handle.net/20.500.12110/paper_00046361_v540_n_p_Piatti
Aporte de:
id paper:paper_00046361_v540_n_p_Piatti
record_format dspace
spelling paper:paper_00046361_v540_n_p_Piatti2023-06-08T14:28:00Z Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud galaxies: individual: LMC galaxies: star clusters: general techniques: photometric Angular sizes Galaxies: individual: LMC Galaxies: star clusters Large magellanic clouds techniques: photometric Washington Galaxies Photometers Stars Photometry Aims. With the aim of enlarging the number of studied LMC clusters in the age range 8.0 ≈ log(t) ≈ 9.0, we focus here on a sample of mostly unstudied cluster candidates. Methods. We present for the first time CCD Washington CT 1T 2 photometry of stars in the field of 26 LMC clusters. Results. The studied clusters turned out to be small angular size objects with ages within the age range 8.0 ≈ log(t) ≈ 9.0, which are projected or immersed in dense star fields. © 2012 ESO. 2012 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v540_n_p_Piatti http://hdl.handle.net/20.500.12110/paper_00046361_v540_n_p_Piatti
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic galaxies: individual: LMC
galaxies: star clusters: general
techniques: photometric
Angular sizes
Galaxies: individual: LMC
Galaxies: star clusters
Large magellanic clouds
techniques: photometric
Washington
Galaxies
Photometers
Stars
Photometry
spellingShingle galaxies: individual: LMC
galaxies: star clusters: general
techniques: photometric
Angular sizes
Galaxies: individual: LMC
Galaxies: star clusters
Large magellanic clouds
techniques: photometric
Washington
Galaxies
Photometers
Stars
Photometry
Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
topic_facet galaxies: individual: LMC
galaxies: star clusters: general
techniques: photometric
Angular sizes
Galaxies: individual: LMC
Galaxies: star clusters
Large magellanic clouds
techniques: photometric
Washington
Galaxies
Photometers
Stars
Photometry
description Aims. With the aim of enlarging the number of studied LMC clusters in the age range 8.0 ≈ log(t) ≈ 9.0, we focus here on a sample of mostly unstudied cluster candidates. Methods. We present for the first time CCD Washington CT 1T 2 photometry of stars in the field of 26 LMC clusters. Results. The studied clusters turned out to be small angular size objects with ages within the age range 8.0 ≈ log(t) ≈ 9.0, which are projected or immersed in dense star fields. © 2012 ESO.
title Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
title_short Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
title_full Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
title_fullStr Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
title_full_unstemmed Washington photometry of 26 moderately young small angular size clusters in the Large Magellanic Cloud
title_sort washington photometry of 26 moderately young small angular size clusters in the large magellanic cloud
publishDate 2012
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v540_n_p_Piatti
http://hdl.handle.net/20.500.12110/paper_00046361_v540_n_p_Piatti
_version_ 1768544019691864064