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The local system of early type stars - Spatial extent and kinematics
Published uvby and H-beta photometric data and proper motions arecompiled and analyzed to characterize the structure and kinematics ofthe bright early-type O-A0 stars in the solar vicinity, with a focus onthe Gould belt. The selection and calibration techniques are explained,and the data are presented in extensive tables and graphs and discussedin detail. The Gould belt stars of age less than 20 Myr are shown togive belt inclination 19 deg to the Galactic plane and node-lineorientation in the direction of Galactic rotation, while the symmetricaldistribution about the Galactic plane and kinematic properties (purecircular differential rotation) of the belt stars over 60 Myr oldresemble those of fainter nonbelt stars of all ages. The unresolveddiscrepancy between the expansion observed in the youngest nearby starsand the predictions of simple models of expansion from a point isattributed to the inhomogeneous distribution of interstellar matter.

Four-colour and H-beta photometry for early type stars in three southern galactic regions
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1980A&AS...41...85L&db_key=AST

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Dades d'Observació i Astrometria

Constel·lació:Circinus
Ascensió Recta:14h53m50.97s
Declinació:-56°00'42.2"
Magnitud Aparent:8.858
Distancia:1190.476 parsecs
Moviment propi RA:-15.3
Moviment propi Dec:-14.4
B-T magnitude:8.814
V-T magnitude:8.855

Catàlegs i designacions:
Noms Propis   (Edit)
HD 1989HD 131105
TYCHO-2 2000TYC 8685-2517-1
USNO-A2.0USNO-A2 0300-22442075
HIPHIP 72890

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