Mass function of Quintuplet cluster (Hussmann+, 2012)

Details Mass function of Quintuplet cluster (Hussmann+, 2012) Mass function of Quintuplet cluster (Hussmann+, 2012)

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..35409057h&link_type=abstract

VizieR On-line Data Catalog: J/A+A/540/A57. Originally published in: 2012A&A...540A..57H

Physics

Clusters: Open, Stars: Early-Type, Proper Motions, Photometry: Infrared, Stars: Masses

Scientific paper

All sources in this catalogue are located within a radius of 0.5pc from the centre of the observed field of view (near source No. 394). The table contains all sources with measured H-, and Ks-band magnitudes and proper motions, i.e. all sources which appear in the colour-magnitude- diagrams of cluster and field (Fig. 8). For stars with magnitudes above the linearity limits, i.e. Ks<11.3mag and H<12.0mag, the stated magnitude and proper motion errors might be underestimated. For each source the cluster membership was assessed based on 1.) its measured proper motion, 2.) its colour and 3.) its spectral type (if contained in the K-band spectral catalogue of Liermann et al. (2009, Cat. J/A+A/494/1137). For designated cluster members initial masses have been determined from 3, 4, 5Myr Padova isochrones (Marigo et al. 2008A&A...482..883M) and a 4Myr Geneva isochrone with enhanced mass loss (Lejeune & Schaerer 2001, Cat. VI/102).
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Mass function of Quintuplet cluster (Hussmann+, 2012) 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 Mass function of Quintuplet cluster (Hussmann+, 2012), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass function of Quintuplet cluster (Hussmann+, 2012) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1381292