INVESTIGADORES
BAUME Gustavo Luis
artículos
Título:
Extinction in the Star Cluster SAI 113 and Galactic Structure in Carina
Autor/es:
G. CARRARO; D. TURNER; D. MAJAESS; G. BAUME; R. GAMEN; J.A. MOLINA LERA
Revista:
ASTRONOMICAL JOURNAL
Editorial:
IOP PUBLISHING LTD
Referencias:
Lugar: Londres; Año: 2017 vol. 153 p. 156 - 166
ISSN:
0004-6256
Resumen:
Photometric CCD UB VIC photometry obtained for 4860 stars surrounding the embedded southern cluster SAI113 (Skiff 8) is used to examine the reddening in the field and derive the distance to the cluster and nearby vanGenderen1. Spectroscopic color excesses for bright cluster stars, photometric reddenings for A3 dwarfs, and dereddening of cluster stars imply that the reddening and extinction laws match results derived for other young clusters in Carina: EU-B EB-V 0.64 and RV 4. SAI113 displays features that may be linked to a history of dynamical interactions among member stars: possible circumstellar reddening and rapid rotation of late B-type members, ringlike features in star density, and a compact core, with most stars distributed randomly across thefield. The group vanGenderen1 resembles a stellar asterism, with potential members distributed randomly across the field. Distances of 3.90±0.19 kpc and 2.49±0.09 kpc are derived for SAI113 and vanGenderen1, respectively, with variable reddenings EB-V ranging from 0.84 to 1.29 and 0.23 to 1.28. The SRC variables CKCar and EVCar may be outlying members of vanGenderen1, thereby of use for calibrating the period?luminosity relation for pulsating M supergiants. More importantly, the anomalous reddening and extinction evidentin Carina and nearby regions of the Galactic plane in the fourth quadrant impact the mapping of spiral structure from young open clusters. The distribution of spiral arms in the fourth quadrant may be significantly different from how it is often portrayed.