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Bogdan Popescu - Publications

Affiliations: 
2006-2010 Department of Physics University of Cincinnati, Cincinnati, OH 
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7 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2014 Borissova J, Chené AN, Ramírez Alegría S, Sharma S, Clarke JRA, Kurtev R, Negueruela I, Marco A, Amigo P, Minniti D, Bica E, Bonatto C, Catelan M, Fierro C, Geisler D, ... ... Popescu B, et al. New galactic star clusters discovered in the VVV survey.Candidates projected on the inner disk and bulge Astronomy and Astrophysics. 569. DOI: 10.1051/0004-6361/201322483  0.649
2013 Popescu B, Hanson MM. The Range Of Variation Of The Mass Of The Most Massive Star In Stellar Clusters Derived From 35 Million Monte Carlo Simulations The Astrophysical Journal. 780: 27. DOI: 10.1088/0004-637X/780/1/27  0.702
2012 Popescu B, Hanson MM, Elmegreen BG. Age And Mass For 920 Large Magellanic Cloud Clusters Derived From 100 Million Monte Carlo Simulations The Astrophysical Journal. 751: 122. DOI: 10.1088/0004-637X/751/2/122  0.718
2010 Popescu B, Hanson MM. MASSCLEANcolors—Mass-dependent Integrated Colors for Stellar Clusters Derived from 30 Million Monte Carlo Simulations The Astrophysical Journal. 713. DOI: 10.1088/2041-8205/713/1/L21  0.723
2010 Popescu B, Hanson MM. MASSCLEANage-STELLAR CLUSTER AGES FROM INTEGRATED COLORS The Astrophysical Journal. 724: 296-305. DOI: 10.1088/0004-637X/724/1/296  0.706
2009 Popescu B, Hanson MM. Massclean—Massive Cluster Evolution And Analysis Package: Description And Tests The Astronomical Journal. 138: 1724-1740. DOI: 10.1088/0004-6256/138/6/1724  0.716
2009 Popescu B, Hanson MM. massclean (MASSive CLuster Evolution and ANalysis Package): description, tests, and results Arxiv: Astrophysics of Galaxies. 5: 511-515. DOI: 10.1017/S1743921309991876  0.726
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