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Pulkovo compilation of radial velocities for 35495 stars in a common system.
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Positional reference stars in the Magellanic Clouds
The equatorial coordinates are determined of 926 stars (mainly ofgalactic origin) in the direction of the Magellanic Clouds at the meanepoch T = 1978.4 with an overall accuracy characterized by the meanvalues of the O-C coordinates, Sa = 0.35 arcsec and Sd = 0.38 arcsec,calculated from the coordinates of the Perth reference stars. Thesevalues are larger than the accuracy expected for primary standard stars.They allow the new positions to be considered as those of reliablesecondary standard stars. The published positions correspond to anunquestionable improvement of the quality of the coordinates provided inthe current catalogs. This study represents an 'astrometric step' in thestarting of a 'Durchmusterung' of the Magellanic Clouds organized by deBoer (1988, 1989).

Sir John Herschel's Observations of Stars in the Small Magellanic Cloud
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Radial velocities of supergiants in the Small Magellanic Cloud
This paper presents the kinematic results of a study, comparing SmallMagellanic Cloud supergiants to galactic supergiants. The stars werechosen from the lists of Florsch (1972a) and Sanduleak (1968). A roughcorrelation is found between the radial velocities of the supergiantsand the radial velocities of neutral hydrogen. In some cases a betterrelation exists with the radial velocities of the H II regions.

Etude DU Petit Nuage de Magellan par la technique DU prisme-objectif de Fehrenbach.
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Dades d'Observació i Astrometria

Constel·lació:Tucana
Ascensió Recta:00h41m35.88s
Declinació:-74°10'37.5"
Magnitud Aparent:9.036
Moviment propi RA:-8.5
Moviment propi Dec:-11.4
B-T magnitude:10.411
V-T magnitude:9.15

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 4067
TYCHO-2 2000TYC 9141-1780-1
USNO-A2.0USNO-A2 0150-00363372
HIPHIP 3268

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