The Vertical Structure of the Halo Rotation

Simple item page
dc.creatorKinman, T. D.
dc.creatorCacciari, C.
dc.creatorBragaglia, A.
dc.creatorBuzzoni, A.
dc.creatorSpagna, A.
dc.date2002-11-12
dc.date.accessioned2026-07-07T02:06:10Z
dc.date.available2026-07-07T02:06:10Z
dc.descriptionNew GSC-II proper motions of RR Lyrae and Blue Horizontal Branch (BHB) stars near the North Galactic Pole are used to show that the Galactic Halo 5 kpc above the Plane has a significantly retrograde galactic rotation.
dc.descriptionPaper presented at the Galactic Dynamics Workshop (JENAM 2002), 6 pages, uses eas.cls (included)
dc.identifierhttps://arxiv.org/abs/astro-ph/0211243
dc.identifierhttp://arxiv.org/abs/astro-ph/0211243
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5329
dc.subjectAstrophysics
dc.titleThe Vertical Structure of the Halo Rotation
dc.typetext

Files

Collections

arXiv