Characterization of the praesepe star cluster by photometry and proper motions with 2MASS, PPMXL, and Pan-STARRS

Astrophysical Journal

Volumn 784, Issue 1, 2014, Pages

  Wang, P F ^a   Chen, W P ^a   Lin, C C ^a   Pandey, A K ^b   Huang, C K ^a   Panwar, N ^a   Lee, C H ^a   Tsai, M F ^a   Tang, C H ^a   Goldman, B ^c   Burgett, W S ^d   Chambers, K C ^d   Draper, P W ^e   Flewelling, H ^d   Grav, T ^f   Heasley, J N ^d   Hodapp, K W ^d   Huber, M E ^d   Jedicke, R ^d   Kaiser, N ^d   Kudritzki, R P ^d   Luppino, G A ^d   Lupton, R H ^g   Magnier, E A ^d   Metcalfe, N ^e   Monet, D G ^h   Morgan, J S ^d   Onaka, P M ^d   Price, P A ^d   Stubbs, C W ⁱ   Sweeney, W ^d   Tonry, J L ^d   Wainscoat, R J ^d   Waters, C ^d   more..

^a NATIONAL CENTRAL UNIVERSITY   (Taiwan)

^b ARYABHATTA RESEARCH INSTITUTE OF OBSERVATIONAL SCIENCES ARIES   (India)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d UNIVERSITY OF HAWAII   (United States)

^e DURHAM UNIVERSITY   (United Kingdom)

^f JOHNS HOPKINS UNIVERSITY   (United States)

^g PRINCETON UNIVERSITY   (United States)

^h FLAGSTAFF STATION   (United States)

ⁱ HARVARD UNIVERSITY   (United States)

Author keywords

open clusters and associations: individual (Praesepe); stars: kinematics and dynamics; stars: luminosity function, mass function

Indexed keywords

EID: 84896755070     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/784/1/57     Document Type: Article

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