OB Stars in the Solar Neighborhood II: Kinematics

Details OB Stars in the Solar Neighborhood II: Kinematics OB Stars in the Solar Neighborhood II: Kinematics

2006-05-17

arxiv.org/abs/astro-ph/0605408v1

Astron.J.132:1052-1060,2006

Astronomy and Astrophysics

Astrophysics

23 pages (including 4 figures). To be published in the Astronomical Journal (accepted May 17th, 2006)

Scientific paper

10.1086/505941

Using the spatial classification method and the structural parameters estimated for the Gould Belt (GB) and the local Galactic disk (LGD) from a previous paper, we have evaluated spatial membership probabilities for a sample of O and B stars from the Hipparcos catalogue (ESA 1997) with available proper motions and radial velocity data. Thus being able to study the space velocity fields of both systems, we conclude that the GB and the LGD present different statistical distributions, both in the velocity space as well as in the phase space. In the light of the existence of both systems we analyze different kinematic aspects in the vicinity of the Sun, and we find the GB to be responsible for the highly negative vertex deviation found for the OB stars in the solar neighborhood. We also find that the GB sensibly alters the estimation of Oort's constants in the Galactic disk; thus, in order to establish comparisons with other kinematic studies based in older stellar populations, a careful pruning of the GB members must be performed. Further analysis of the GB velocity field and the moving groups that contribute to it suggest the possibility that the GB can be the result of a chance superposition of moving groups. We propose for future investigations the dynamical analysis of these moving groups in order to probe the origin of the GB.

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