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New proper motion members of Cygnus OB2 - Other overdensities: Right over-density proper motion members and Left over-density proper motion members
Gaia DR2 five astrometric parameters and magnitude of the proper motion members of the association Cygnus OB2 and of the substructures named 'Right over-density' and 'Left over-density' are presented. For each group the ...
PROPER-MOTION SURVEY .1. COMMON-PROPER-MOTION SYSTEMS IN ESO AREAS 439 AND 440
(AMER INST PHYSICS, 1990-03)
High proper motion stars with declinations between −30° and −40° , and right ascensions between 00 h and 10 h 40m
(2001)
Proper motions, positions, nding charts and magnitudes are given for 147 newly discovered stars with
proper motions larger than 0.15 arcsec/year. They were found in a search for high proper motion stars carried out
in ...
Kinematic parameters and membership probabilities of open clusters in the Bordeaux PM2000 catalogue
(EDP SCIENCES S A, 2010)
Aims. We derive lists of proper-motions and kinematic membership probabilities for 49 open clusters and possible open clusters in the zone of the Bordeaux PM2000 proper motion catalogue (+ 11 degrees <= delta <= + 18 ...
New high proper motion stars with declinations between −5° and −30° , and right ascensions between 13h 30m and 24h
(1999)
Proper motions, positions, nding charts and
magnitudes are given for 293 newly discovered stars with
proper motions larger than 0.15 arcsec/year. They are located
between −5 and −30 in declination, and 13h 30m
and ...
Proper motion of the Large Magellanic Cloud using QSOs as an inertial reference system: The Q0459-6427 field
(2002-04)
The proper motion of the Large Magellanic Cloud relative to one background quasi-stellar object is determined
using 44 CCD frames obtained from 1989.0 to 2000.0 at the Cassegrain focus of the Cerro Tololo
Inter-American ...
Proper motions of the optically visible open clusters based on the UCAC4 catalog
(EDP SciencesLes Ulis, 2014)
We present a catalog of mean proper motions and membership probabilities of individual stars for optically visible open clusters,
which have been determined using data from the UCAC4 catalog in a homogeneous way. The mean ...