VLT/VIMOS Integral field kinematics of the Giant Low Surface Brightness galaxy ESO 323-G064

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dc.creatorCoccato, L.
dc.creatorSwaters, R.
dc.creatorRubin, V. C.
dc.creatorD'Odorico, S.
dc.creatorMcGaugh, S.
dc.date2007-11-28
dc.date.accessioned2026-07-07T08:45:49Z
dc.date.available2026-07-07T08:45:49Z
dc.descriptionWe studied the bulge and the disk kinematic of the giant Low Surface Brightness (LSB) galaxy ESO 323-G064 in order to investigate its dynamics and its Dark Matter (DM) content. We observed the galaxy with the integral field spectroscopy (VLT/VIMOS, in IFU configuration). Results for the gaseous kinematics (bulge and disk) and stellar kinematics (bulge) are presented, together with a Jeans model for the stellar bulge kinematics.
dc.descriptionProceeding of Formation and evolution of galaxy disks, 1-5 Oct. 2007, Rome - Italy
dc.identifierhttps://arxiv.org/abs/0711.4466
dc.identifierhttp://arxiv.org/abs/0711.4466
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143083
dc.subjectAstrophysics
dc.titleVLT/VIMOS Integral field kinematics of the Giant Low Surface Brightness galaxy ESO 323-G064
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