J/MNRAS/434/3236    Masses of Praesepe members                   (Khalaj+, 2013)

The stellar mass function, binary content and radial structure of the open cluster Praesepe derived from PPMXL and SDSS data. Khalaj P., Baumgardt H. <Mon. Not. R. Astron. Soc., 434, 3236-3245 (2013)> =2013MNRAS.434.3236K 2013MNRAS.434.3236K
ADC_Keywords: Clusters, open ; Proper motions ; Photometry, infrared ; Stars, masses Keywords: stars: luminosity function, mass function - open clusters and associations: individual: Praesepe Abstract: We have determined possible cluster members of the nearby open cluster Praesepe (M44) based on J and K photometry and proper motions from the PPMXL catalogue and z photometry from the Sloan Digital Sky Survey. In total, we identified 893 possible cluster members down to a magnitude of J=15.5mag, corresponding to a mass of about 0.15M for an assumed cluster distance modulus of (m-M)0=6.30mag (d∼182pc), within a radius of 3.5° around the cluster centre. We derive a new cluster centre for Praesepe (RAcentre=8:39:37, DEcentre=19:35:02). We also derive a total cluster mass of about 630M, and a 2D half-number and half-mass radius of 4.25 and 3.90pc, respectively. Description: In this study, we combine data from the PPMXL catalogue (Roser et al., 2010AJ....139.2440R 2010AJ....139.2440R, Cat. I/317) with z magnitudes from SDSS DR9 (Ahn et al., 2012ApJS..203...21A 2012ApJS..203...21A, Cat. V/139). The PPMXL catalogue combines the USNO-B1.0 (Monet et al. 2003AJ....125..984M 2003AJ....125..984M, Cat. I/284) and 2MASS catalogues (Skrutskie et al. 2006AJ....131.1163S 2006AJ....131.1163S, Cat. VII/233), yielding the largest collection of proper motions in the International Celestial Reference Frame to date (Roser et al., 2010AJ....139.2440R 2010AJ....139.2440R, Cat. I/317). Cat. J/A+A/531/A92). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 73 893 Celestial coordinates, proper motions, magnitudes and the masses of the possible members of Praesepe sorted by right ascension -------------------------------------------------------------------------------- See also: I/257 : Proper Motions in Praesepe (Wang+, 1995) I/284 : The USNO-B1.0 Catalog (Monet+ 2003) I/317 : PPMXL Catalog (Roeser+ 2010) V/139 : SDSS Photometric Catalog, DR 9 (Adelman-McCarthy+, 2012) VII/233 : 2MASS Extended sources (IPAC/UMass, 2003-2006) J/AJ/134/2340 : Membership of Praesepe & Coma Berenices clusters (Kraus+, 2010) J/MNRAS/426/3419 : UKIDSS GCS Praesepe members (Boudreault+, 2012) J/MNRAS/442/2081 : Praesepe members light curves (Kovacs+, 2014) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.6 deg RAdeg Right Ascension (J2000) (1) 12- 21 F10.6 deg DEdeg Declination (J2000) (1) 23- 27 F5.1 mas/yr pmRA Proper motion in RA (pmRA*cos(DE)) (1) 29- 31 F3.1 mas/yr e_pmRA Error of pmRA (1) 33- 37 F5.1 mas/yr pmDE Proper Motion in Dec (1) 39- 41 F3.1 mas/yr e_pmDE Error of pmDE (1) 43- 48 F6.3 mag Jmag 2MASS J magnitude (1) 50- 54 F5.3 mag e_Jmag Error of Jmag (1) 56- 61 F6.3 mag Kmag 2MASS Ks magnitude (1) 63- 67 F5.3 mag e_Kmag Error of Kmag (1) 69- 73 F5.3 Msun Mass Mass (2) -------------------------------------------------------------------------------- Note (1): All data are from PPMXL Note (2): Stellar masses are derived by J magnitudes using PADOVA isochornes. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 15-Sep-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line