Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Neelam Panwar"'
The evolution of HII regions/supershells can trigger a new generation of stars/clusters at their peripheries, with environmental conditions that may affect the initial mass function, disk evolution and star formation efficiency. In this paper we stud
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d3e04d727c8b1e7b8bcb0f1b68f0505
Our star-count analysis of the Two Micron All Sky Survey point sources resulted in an identification of the star cluster G144.9+0.4. The cluster was found, but not characterized, by Glushkova et al. We show that the cluster is physically associated w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a539b96dcc28ca3186d65cef5bd0a703
Publikováno v:
AIP Conference Proceedings.
Open clusters are good laboratories to study stellar evolution and dynamical interaction among member stars. We are carrying out a program to identify uncharted clusters using sky-survey data. Our preliminary result is finding stellar density enhance
Autor:
Christopher W. Stubbs, J. N. Heasley, Chien-Hsiu Lee, Robert Jedicke, Robert H. Lupton, Paul A. Price, Gerard Anthony Luppino, Tommy Grav, C. K. Huang, W. P. Chen, Richard J. Wainscoat, Peter M. Onaka, William S. Burgett, Mengchun Tsai, R. P. Kudritzki, K. C. Chambers, Klaus W. Hodapp, J. S. Morgan, John L. Tonry, C. H. Tang, Mark E. Huber, Ping Wang, Nick Kaiser, Neelam Panwar, Nigel Metcalfe, H. Flewelling, Peter W. Draper, E. A. Magnier, Bertrand Goldman, Christopher Waters, Chien-Cheng Lin, W. E. Sweeney, Ashwani Pandey, David G. Monet
Publikováno v:
Astrophysical journal, 2014, Vol.784(1), pp.57 [Peer Reviewed Journal]
Membership identification is the first step to determine the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history, such as mass segregation, stellar evaporation, or tidal stripping, of a star clust