arXiv Analytics

Sign in

arXiv:1309.0608 [astro-ph.GA]AbstractReferencesReviewsResources

Search for and Characterization of Open Clusters Toward the Galactic Anti-center with Pan-STARRS1

C. C. Lin, W. P. Chen

Published 2013-09-03Version 1

We have used a star-count algorithm based the Panoramic Survey Telescope And Rapid Response System 3$\pi$ survey data aim to identify and characterize uncharted open clusters (OCs). With limiting magnitudes of about 22 mag in \gps, \rps, \ips\ bands and about 20 mag in \zps\ and \yps\ bands, our data are 100 times more sensitive than currently available surveys. We analyzed a trial region within $20\deg\times20\deg$ field toward the Galactic anticenter and found 1660 density enhancement regions of which 79 (out of 129) are known OCs, and 949 are OC candidates.

Comments: 6 pages, 6 eps figures, paper presented at the 10th Pacific Rim Conference on Stellar Astrophysics, Seoul, May 27-31, 2013, ASP Conference Series, in press
Categories: astro-ph.GA
Related articles: Most relevant | Search more
arXiv:2305.10001 [astro-ph.GA] (Published 2023-05-17)
Investigating kinematics and dynamics of three open clusters towards Galactic anti-center
arXiv:0910.1478 [astro-ph.GA] (Published 2009-10-08)
The spatial distribution of stars in open clusters
arXiv:2209.01738 [astro-ph.GA] (Published 2022-09-05)
Stellar Population Astrophysics (SPA) with the TNG. alpha-elements, lithium, sodium and aluminum in 16 open clusters
R. Zhang et al.