dc.creator | Baume, Gustavo Luis | |
dc.creator | Moitinho, A. | |
dc.creator | Vázquez, Rubén Ángel | |
dc.creator | Solivella, Gladys Rebeca | |
dc.creator | Carraro, G. | |
dc.creator | Villanova, S. | |
dc.date | 2006 | |
dc.date | 2019-11-04T18:30:34Z | |
dc.identifier | http://sedici.unlp.edu.ar/handle/10915/84880 | |
dc.identifier | issn:0035-8711 | |
dc.description | Based on a deep optical CCD [<i>UBV(RI)</i><SUB>C</SUB>] photometric survey and on the Two-Micron All Sky Survey (2MASS) data, we derived the main parameters of the open cluster NGC 2401. We found that this cluster is placed at 6.3 ± 0.5 kpc (V<SUB>o</SUB> - M<SUB>v</SUB> = 14.0 ± 0.2) from the Sun and is 25 Myr old, which allows us to identify NGC 2401 as a member of the young population belonging to the innermost side of the extension of the Norma-Cygnus spiral arm in the Third Galactic Quadrant. A spectroscopic study of the emission star LSS 440 that lies in the cluster area revealed that it is a B0Ve star; however, we could not confirm that it is a cluster member. We also constructed the cluster luminosity function (LF) down to V ∼ 22 and the cluster initial mass function (IMF) for all stars with masses above M ∼ 1-2 M ⊙. It was found that the slope of the cluster IMF is x ≈ 1.8 ± 0.2. The presence of a probable pre-main-sequence (PMS) star population associated with the cluster is weakly revealed. | |
dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
dc.description | Instituto de Astrofísica de La Plata | |
dc.format | application/pdf | |
dc.format | 1441-1449 | |
dc.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
dc.subject | Ciencias Astronómicas | |
dc.subject | Galaxy: structure | |
dc.subject | Open clusters and associations: individual: NGC 2401 | |
dc.subject | Stars: emission-line, Be | |
dc.subject | Stars: imaging | |
dc.subject | Stars: individual: LSS 440 | |
dc.subject | Stars: luminosity function, mass function | |
dc.title | NGC 2401: A template of the young population of the Norma-Cygnus arm in the Third Galactic Quadrant | |
dc.type | Articulo | |
dc.type | Articulo | |