arXiv Analytics

Sign in

arXiv:1606.01958 [astro-ph.SR]AbstractReferencesReviewsResources

Stellar populations in the Carina region: The Galactic plane at l = 291

J. A. Molina-Lera, G. Baume, R. Gamen, E. Costa, G. Carraro

Published 2016-06-06Version 1

Previous studies of the Carina region have revealed its complexity and richness as well as a significant number of early-type stars. In many cases, these studies only concentrated on the central region or were not homogeneous. This latter aspect, in particular, is crucial because very different ages and distances for key clusters have been claimed in recent years. The aim of this work is to study in detail an area of the Galactic plane in Carina. We analyze the properties of different stellar populations and focus on a sample of open clusters and their population of YSOs and highly reddened early stars. We also studied the stellar mass distribution in these clusters and the possible scenario of their formation. Finally, we outline the Galactic spiral structure in this direction. We obtained photometric data for six young open clusters located in Carina at l = 291, and their adjacent stellar fields, which we complemented with spectroscopic observations of a few selected targets. We also culled additional information from the literature. Our results provide more reliable estimates of distances, color excesses, masses, and ages of the stellar populations in this direction. We estimate the basic parameters of the studied clusters and find that they identify two overdensities of young stellar populations. We find evidence of PMS populations inside them, with an apparent coeval stellar formation in the most conspicuous clusters. We also discuss apparent age and distance gradients in the direction NW-SE. We study the mass distributions of several clusters in the region. They consistently show a canonical IMF slope. We discover and characterise an abnormally reddened massive stellar population. Spectroscopic observations of ten stars of this latter population show that all selected targets were massive OB stars. Their location is consistent with the position of the Car-Sag spiral arm.

Related articles: Most relevant | Search more
arXiv:2412.05356 [astro-ph.SR] (Published 2024-12-06)
The Mass Distribution of Stars Stripped in Binaries: The Effect of Metallicity
arXiv:1511.07145 [astro-ph.SR] (Published 2015-11-23)
The ATLASGAL survey: distribution of cold dust in the Galactic plane. Combination with Planck data
T. Csengeri et al.
arXiv:1902.05753 [astro-ph.SR] (Published 2019-02-15)
Ruprecht 147 DANCe I. Members, empirical isochrone, luminosity and mass distributions
J. Olivares et al.