Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010)

Details Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010) Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010)

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74082457b&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/408/2457. Originally published in: 2010MNRAS.408.2457B

Mathematics

Probability

Clusters: Open, Photometry: Infrared, Proper Motions

Scientific paper

Presented are the results of a large and deep optical-near-infrared multi-epoch survey of the Praesepe open star cluster using data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Clusters Survey. Multiple colour-magnitude diagrams were used to select potential members and proper motions were used to assign levels of membership probability. From our sample, 145 objects were designated as high probability members (p>=0.6) with most of these having been found by previous surveys although 14 new cluster members are also identified. Our membership assignment is restricted to the bright sample of objects (Z<18). From the fainter sample, 39 candidates were found from an examination of multiple colour-magnitude plots.
(3 data files).

Affiliated with

Also associated with

No associations

Rating

Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-mass stars and brown dwarfs in Praesepe (Baker+, 2010) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1004061