/ftp/cats/J_A+A/329/101



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J/A+A/329/101       Masses of Pleiades members (Raboud+ 1998)
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	table3
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Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+A/329/101
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drwxr-xr-x 9 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jun 16 11:03 [TAR file] -rw-r--r-- 1 cats archive 446 Jan 16 1998 .message -r--r--r-- 1 cats archive 4131 Jan 16 1998 ReadMe -rw-r--r-- 1 cats archive 213 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2047 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 6447 Aug 26 1997 table3.gz [Uncompressed]
Beginning of ReadMe : J/A+A/329/101 Masses of Pleiades members (Raboud+ 1998) ================================================================================ Investigation of the Pleiades cluster. IV. The radial structure. Raboud D., Mermilliod J.-C. <Astron. Astrophys. 329, 101 (1998)> =1998A&A...329..101R (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Clusters, open ; Stars, masses Keywords: cluster: open: individual: Pleiades - binary: spectroscopic Abstract: On the basis of the best available member list and duplicity information, we have studied the radial distribution of 270 stars and multiple systems earlier than K0 in the Pleiades. Five new long period spectroscopic binaries have been identified from the CORAVEL observations. We have found a clear mass segregation between binaries and single stars, which is explained by the greater average mass of the multiple systems. The mass function of the single stars and primaries appears to be significantly different. While the central part of the cluster is spherical, the outer part is clearly elliptical, with an ellipticity of 0.17. The various parameters describing the Pleiades are (for a distance of 125pc): core radius r_c_=0.6 deg (1.4pc), tidal radius r_t_=7.4 (16pc), half mass radius r_m/2_=0.88 (1.9pc), harmonic radius r=1.82 (4pc). Low-mass stars (later than K0) probably extend further out and new proper motion and radial velocity surveys over a larger area and to fainter magnitudes would be very important to improve the description of the cluster structure and complete mass function. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 03 47.0 +24 07 Pleiades = Cl Melotte 22 ----------------------------------------------------------

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