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23 April 2024
 
  » arxiv » astro-ph/0012386

 Article overview


The consequences of ram pressure stripping on the Virgo cluster spiral galaxy NGC 4522
B. Vollmer ; M. Marcelin ; P. Amram ; C. Balkowski ; V. Cayatte ; O. Garrido ;
Date 18 Dec 2000
Subject astro-ph
Affiliation1,3), M. Marcelin , P. Amram , C. Balkowski , V. Cayatte , O. Garrido ( Observatoire de Paris, France, Observatoire de Marseille, France, ITA Heidelberg, Germany
AbstractNew 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.
Source arXiv, astro-ph/0012386
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