The consequences of ram pressure stripping on the Virgo cluster spiral galaxy NGC 4522

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dc.creatorVollmer, B.
dc.creatorMarcelin, M.
dc.creatorAmram, P.
dc.creatorBalkowski, C.
dc.creatorCayatte, V.
dc.creatorGarrido, O.
dc.date2000-12-18
dc.date.accessioned2026-07-07T01:57:05Z
dc.date.available2026-07-07T01:57:05Z
dc.descriptionNew H-alpha Fabry-Perot interferometer observations of the Virgo cluster spiral galaxy NGC 4522 are presented. A velocity field up to a radius of 60'' was obtained. The observed rotation curve is symmetric. It is not perturbed in the inner disk. For radii >50'' it shows a solid body rotation. We compare these data with a numerical model which includes the effects of ram pressure stripping. The model can reproduce the main characteristics of the H-alpha emission distribution and velocity field. We therefore conclude that the stripping event which caused the HI deficiency and the distorted H-alpha distribution and velocity field has been due to ram pressure. The closest passage of the galaxy to the cluster center is estimated to be approx. 6.5 10^8 yr ago. The observed recent star formation is due to the re-accretion of gas clouds which were accelerated to velocities below the escape velocity during the stripping event. Furthermore, the gas which is located at radii >60'' is part of an asymmetric expanding ring of gas clouds. A substantial part of these clouds is located above the disk plane. We predict the HI gas distribution and velocity field as it would be observed by deep 21 cm observations.
dc.description11 pages with 11 figures, A&A, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0012386
dc.identifierhttp://arxiv.org/abs/astro-ph/0012386
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2245
dc.subjectAstrophysics
dc.titleThe consequences of ram pressure stripping on the Virgo cluster spiral galaxy NGC 4522
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