HST proper motions on the far side of the Galactic bar-data

dc.contributor.authorSoto, Mario, Kuijken, Konrad, Rich, R. Michael, Clarkson, William, I, Castellon, Jose Luis Nilo, Fernandez-Trincado, Jose G., Ramos, Rodrigo Contreras, Kunder, Andrea, Baravalle, Laura D., Alonso, M. Victoria, Simion, Iulia T., Johnson, Christian, I, Vieira, Katherine
dc.date.accessioned2024-11-27T21:50:37Z
dc.date.available2024-11-27T21:50:37Z
dc.date.issued2023/07/04
dc.description.abstractThis is the third paper in a series that attempts to observe a clear signature of the Galactic bar/bulge using kinematic observations of the bulge stellar populations in low foreground extinction windows. We report on the detection of & SIM,100 000 new proper motions in four fields covering the far side of the Galactic bar/bulge, at negative longitudes. Our proper motions have been obtained using observations from the Advance Camera for Surveys (ACS), on board of the Hubble Space Telescope (HST), with a time-baseline of 8-9 years, which has produced accuracies better than 0.5 mas yr(-1) for a significant fraction of the stellar populations with F814W < 23 mag. Interestingly, as shown in previous works, the Hess diagrams show a strikingly similar proper motion distribution to fields closer to the Galactic center and consistent with an old stellar population. The observed kinematics point to a significant bulge rotation, which seems to predominate even in fields as far as l & SIME, -8 & DEG,, and is also reflected in the changes of the velocity ellipsoid in the l, b plane as a function of distance.
dc.identifier.doihttp://dx.doi.org/10.1093/mnras/stad1911
dc.identifier.issn0035-8711
dc.identifier.urihttps://publicacionesabiertas.userena.cl/handle/123456789/113
dc.languageEnglish
dc.publisherOXFORD UNIV PRESS
dc.subjectMILKY-WAY BULGE, STELLAR POPULATIONS, VERTEX DEVIATION, RED CLUMP, KINEMATICS, VVV, AGE, ABUNDANCES, BAR/BULGE, FIELDS
dc.titleHST proper motions on the far side of the Galactic bar-data
dc.typeArticle

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