Skip to main content

Research Repository

Advanced Search

Multiple kinematical populations in Vela OB2 from Gaia DR1 data

Damiani, F.; Prisinzano, L.; Jeffries, R.D.; Sacco, G.G.; Randich, S.; Micela, G.

Multiple kinematical populations in Vela OB2 from Gaia DR1 data Thumbnail


Authors

F. Damiani

L. Prisinzano

G.G. Sacco

S. Randich

G. Micela



Abstract

Context. Recent results using radial-velocity measurements from the Gaia-ESO Survey have led to the discovery of multiple kinematic populations across the Vela OB2 association. We present here a proper-motion study of the same region.
Aims. Our aim is to test whether or not the radial-velocity populations have a counterpart in proper-motion space, and if so, how the two sets of kinematical data complement each other.
Methods. This work is based on parallaxes and proper motions from the TGAS catalogue, as part of Gaia DR1.
Results. Two distinct proper-motion populations are found dispersed across ~ 5 degrees (or ~ 30 pc at their likely distances). Their detailed correspondence to the radial-velocity populations could not be tested because of the paucity of common objects. However, compelling indications are found that one of the new proper-motion populations consists mostly of members of the young cluster NGC 2547, and the other is related to the 2 Vel cluster. Constraints on the age of the two populations, both of which appear to be only 10

Journal Article Type Article
Acceptance Date May 10, 2017
Online Publication Date May 30, 2017
Publication Date 2017-06
Publicly Available Date Mar 29, 2024
Journal Astronomy and Astrophysics
Print ISSN 2329-1273
Publisher Hans Publishers
Peer Reviewed Peer Reviewed
Volume 602
Pages L1 - L1
DOI https://doi.org/10.1051/0004-6361/201730867
Keywords open clusters and associations, individual, Vel OB2, proper motions
Publisher URL https://doi.org/10.1051/0004-6361/201730867

Files




You might also like



Downloadable Citations