A deep and wide-field view at the IC 2944/2948 complex in Centaurus

We employed the ESO Max Planck Institute (MPI) wide-field camera (Baade et al.) and obtained deep images in the VIC pass-bands in the region of the IC 2944/2948 complex (l ~ 294.°8; b ~ -1.°6), and complemented them with literature and archival data. We used this material to derive the photometric,...

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Detalles Bibliográficos
Autores principales: Baume, Gustavo Luis, Rodríguez, María Jimena, Corti, Mariela Alejandra, Carraro, G., Panei, Jorge Alejandro
Formato: Articulo
Lenguaje:Inglés
Publicado: 2014
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85266
Aporte de:
id I19-R120-10915-85266
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
Galaxy: structure
Open clusters and associations: general
Open clusters and associations: individual: IC 2944
Stars: early-type
Stars: formation
Stars: pre-main-sequence
spellingShingle Ciencias Astronómicas
Galaxy: structure
Open clusters and associations: general
Open clusters and associations: individual: IC 2944
Stars: early-type
Stars: formation
Stars: pre-main-sequence
Baume, Gustavo Luis
Rodríguez, María Jimena
Corti, Mariela Alejandra
Carraro, G.
Panei, Jorge Alejandro
A deep and wide-field view at the IC 2944/2948 complex in Centaurus
topic_facet Ciencias Astronómicas
Galaxy: structure
Open clusters and associations: general
Open clusters and associations: individual: IC 2944
Stars: early-type
Stars: formation
Stars: pre-main-sequence
description We employed the ESO Max Planck Institute (MPI) wide-field camera (Baade et al.) and obtained deep images in the VIC pass-bands in the region of the IC 2944/2948 complex (l ~ 294.°8; b ~ -1.°6), and complemented them with literature and archival data. We used this material to derive the photometric, spectroscopic and kinematic properties of the brightest (V < 16) stars in the region. The VI deep photometry on the other end, helped us to unravel the lower main sequence of a few, possibly physical, star groups in the area. Our analysis confirmed previous suggestions that the extinction towards this line of sight follows the normal law (RV = 3.1). We could recognize B-type stars spread in distance from a few hundred pc to at least 2 kpc. We found two young groups (age ~ 3 Myr) located, respectively, at about 2.3 and 3.2 kpc from the Sun. They are characterized by a significant variable extinction (E(B - V) ranging from 0.28 to 0.45 mag), and host a significant pre-main-sequence population. We computed the initial mass functions for these groups and obtained slopes G{cyrillic} from -0.94 to -1.02 (eG{cyrillic} = 0.3) in a scale where the classical Salpeter law is -1.35. We estimated the total mass of bothmain stellar groups in ~ 1100 and ~ 500M⊙, respectively. Our kinematic analysis indicated that both groups of stars deviate from the standard rotation curve of the Milky Way, in line with literature results for this specific Galactic direction. Finally, along the same line of sight, we identified a third group of early-type stars located at ~8 kpc from the Sun. This group might be located in the far side of the Sagittarius-Carina spiral arm.
format Articulo
Articulo
author Baume, Gustavo Luis
Rodríguez, María Jimena
Corti, Mariela Alejandra
Carraro, G.
Panei, Jorge Alejandro
author_facet Baume, Gustavo Luis
Rodríguez, María Jimena
Corti, Mariela Alejandra
Carraro, G.
Panei, Jorge Alejandro
author_sort Baume, Gustavo Luis
title A deep and wide-field view at the IC 2944/2948 complex in Centaurus
title_short A deep and wide-field view at the IC 2944/2948 complex in Centaurus
title_full A deep and wide-field view at the IC 2944/2948 complex in Centaurus
title_fullStr A deep and wide-field view at the IC 2944/2948 complex in Centaurus
title_full_unstemmed A deep and wide-field view at the IC 2944/2948 complex in Centaurus
title_sort deep and wide-field view at the ic 2944/2948 complex in centaurus
publishDate 2014
url http://sedici.unlp.edu.ar/handle/10915/85266
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