Deep optical survey of the stellar content of Sh2-311 region

Abstract

The stellar content in and around Sh2-311 region have been studied using the deep optical observations as well as near-infrared (NIR) data from 2MASS. The region contains three clusters, viz. NGC 2467, Haffner 18 and Haffner 19. We have made an attempt to distinguish the stellar content of these individual regions as well as to re-determine their fundamental parameters such as distance, reddening, age, onto the basis of a new and more extended optical and infrared photometric data set. NGC 2467 and Haffner 19 are found to be located in the Perseus arm at the distances of 5.0 $\pm$ 0.4 kpc and 5.7 $\pm$ 0.4 kpc, respectively, whereas Haffner 18 is located at the distance of 11.2 $\pm$ 1.0 kpc. The clusters NGC 2467 and Haffner 19 might have formed from the same molecular cloud, whereas the cluster Haffner 18 is located in the outer galactic arm, i.e. the Norma-Cygnus arm. We identify 8 class II young stellar objects (YSOs) using the NIR $(J-H)/(H-K)$ two colour diagram. We have estimated the age and mass of the YSOs identified in the present work and those by Snider et al. (2009) using the $V/(V-I)$ colour-magnitude diagram. The estimated ages and mass range of the majority of the YSOs are $\lesssim$1 Myr and $\sim$0.4 - 3.5 \msun, respectively, indicating that these sources could be T-Tauri stars or their siblings. Spatial distribution of the YSOs shows that some of the YSOs are distributed around the H II region Sh2-311, suggesting a triggered star formation at its periphery.

arXiv comment19 pages, 13 figures, 9 table; Accepted for publication in New Astronomy

References in corpus (20)

• Evolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models
• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting observed SEDs using a large grid of pre-computed models
• Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDs
• The Complete Census of 70-um-Bright Debris Disks within the FEPS (Formation and Evolution of Planetary Systems) Spitzer Legacy Survey of Sun-like Stars
• HII Region Metallicity Distribution in the Milky Way Disk
• Binarity as a key factor in protoplanetary disk evolution: Spitzer disk census of the eta Chamaeleontis cluster
• Wide Field CCD photometry around nine open clusters
• T Tauri candidates and accretion rates using IPHAS: method and application to IC1396
• Morphology of Galactic Open Clusters
• Triggered Star Formation in the Orion Bright-Rimmed Clouds
• Triggered Star Formation and Evolution of T-Tauri stars in and around Bright-Rimmed Clouds
• Detection of a young stellar population in the background of open clusters in the Third Galactic Quadrant
• Stellar contents and star formation in the young star cluster Be 59
• Star formation in bright-rimmed clouds and cluster associated with W5 E H{\sc ii} region
• Interstellar extinction in the open clusters towards galactic longitude around 130 degrees
• Optical photometric and polarimetric investigation of NGC 1931
• Spitzer Observations of the HII Region NGC 2467: An Analysis of Triggered Star Formation
• The population in the background of open clusters: Tracer of the Norma-Cygnus arm
• Pre-main-sequence population in NGC 1893 region
• UBVRI photometry and spectroscopy of the young open cluster Haffner 18

Cited by in corpus (5)

• The Villafranca catalog of Galactic OB groups: I. Systems with O2-O3.5 stars
• The massive multiple system HD 64315
• A multiwavelength investigation of the HII region S311: Young stellar population and star formation
• History of Globulettes in the Milky Way
• Investigating star formation scenarios in the Milky Way using YSO distributions -- A pilot study