UPDATE ON THE NATURE OF VIRGO OVERDENSITY

We use the Eighth Data Release of Sloan Digital Sky Survey catalog with its additional sky coverage of the southern Galactic hemisphere to measure the extent and to study the nature of the Virgo Overdensity (VOD). Hie data show that the VOD extends over no less than 2000 deg super(2), with its true...

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Bibliographic Details
Published in:The Astronomical journal 2012-05, Vol.143 (5), p.1-8
Main Authors: BONACA, ANA, Juric, Mario, Ivezic, Zeljko, Bizyaev, Dmitry, Brewington, Howard, MALANUSHENKO, ELENA, MALANUSHENKO, VIKTOR, ORAVETZ, DANIEL, Pan, Kaike, Shelden, Alaina, Simmons, Audrey, Snedden, Stephanie
Format: Article
Language:English
Subjects:
Aircraft detection
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Ellipsoids
Galactic halos
Hemispheres
MILKY WAY
ORBITS
Sky surveys (astronomy)
STARS
SYMMETRY
Vacuum oxygen decarburizing
Video on demand
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Summary:We use the Eighth Data Release of Sloan Digital Sky Survey catalog with its additional sky coverage of the southern Galactic hemisphere to measure the extent and to study the nature of the Virgo Overdensity (VOD). Hie data show that the VOD extends over no less than 2000 deg super(2), with its true extent likely closer to 3000 deg super(2). We test whether the VOD can be attributed to a tilt in the stellar halo ellipsoid with respect to the plane of the Galactic disk and find that the observed symmetry of the north-south Galactic hemisphere star counts excludes this possibility. We argue that the Virgo Overdensity, in spite of its wide area and cloud-like appearance, is still best explained by a minor merger. Its appearance and position are qualitatively similar to a near perigalacticon merger event and, assuming that the VOD and the Virgo Stellar Stream (VSS) share the same progenitor, consistent with the VSS orbit determined by Casetti-Dinescu et al.
ISSN:0004-6256
1538-3881
1538-3881
DOI:10.1088/0004-6256/143/5/105