J/other/A+AT/25.185  Absolute proper motions of globular clusters (Dambis, 2006)

Absolute proper motions of globular clusters. Dambis A.K. <Astron. Astrophys. Trans., 25, 185-188 (2006)> =2006A&AT...25..185D 2006A&AT...25..185D
ADC_Keywords: Stars, variable; Binaries, eclipsing; Combined data Keywords: Globular clusters - Milky Way - Proper motions - Kinematics Abstract: The absolute proper motions for a total of 92 globular clusters of the Milky Way (60% of all clusters included in the catalogue published by Harris, 1996, Cat. VII/195) are inferred from the UCAC2 proper motions of their likely member stars. The median formal error of the cluster proper motions is equal to 0.8marcsec/yr in both right ascension and declination, whereas the proper-motion errors of individual clusters range from 0.2 to 3marcsec/yr. Tests performed demonstrate the overall validity of the cluster motions; the resulting transverse velocities remain, on the average, virtually constant out to a heliocentric distance of 15kpc and the full space velocity of most of the clusters relative to the Galactic centre remains, on the average, unchanged near 190km/s out to a Galactocentric distance of about 20kpc, in agreement with the overall isothermal structure of the Galactic halo. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 56 92 Proper motions of globular clusters -------------------------------------------------------------------------------- See also: VII/195 : Globular Clusters in the Milky Way (Harris, 1996) J/PAZh/25/10 : Young open clusters space-age distribution (Dambis, 1999) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name Cluster name 10- 20 A11 --- OName Other cluster name 26- 31 F6.2 mas/yr pmRA Proper motion in right ascension 36- 39 F4.2 mas/yr e_pmRA Error of proper motion in right ascension 43- 48 F6.2 mas/yr pmDE Proper motion in declination 53- 56 F4.2 mas/yr e_pmDE Error of proper motion in declination -------------------------------------------------------------------------------- Acknowledgements: Andrei Dambis, dambis(at)yandex.ru
(End) Andrei Dambis [SAI, Russia], Patricia Vannier [CDS] 03-Feb-2014
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