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24 January 2022
 
  » arxiv » astro-ph/0102200

 Article overview


HI deficiency in the galaxy cluster ACO 3627. ATCA observations in the Great Attractor region
B. Vollmer ; V. Cayatte ; W. van Driel ; P.A. Henning ; R.C. Kraan-Korteweg ; C. Balkowski ; P.A. Woudt ; W. Duschl ;
Date 12 Feb 2001
Subject astro-ph
Affiliation1,2,8), V. Cayatte , W. van Driel (1,3), P.A. Henning , R.C. Kraan-Korteweg (1,5), C. Balkowski , P.A. Woudt (6,7), and W. Duschl (2,8) ( DAEC, Observatoire de Paris, France, ITA, Univ. Heidelberg, Germany, Unite Scientifique Nancay, Observatoire de
AbstractATCA 21 cm HI observations of the rich galaxy cluster ACO 3627 in the Great Attractor region are presented. Three fields of 30’ diameter located within one Abell radius of ACO 3627 were observed with a resolution of 15’’ and an rms noise of sim 1 mJy/beam. Only two galaxies were detected in these fields. We compare their HI distribution to new optical R-band images and discuss their velocity fields. The first galaxy is a gas-rich unperturbed spiral whereas the second shows a peculiar HI distribution. The estimated 3-sigma HI mass limit of our observations is sim 7 x 10^8 M_{odot} for a line width of 150 km s^{-1}. The non-detection of a considerable number of luminous spiral galaxies indicates that the spiral galaxies are HI deficient. The low detection rate is comparable to the HI deficient Coma cluster (Bravo-Alfaro et al. 2000). ACO 3627 is a bright X-ray cluster. We therefore suspect that ram pressure stripping is responsible for the HI deficiency of the bright cluster spirals.
Source arXiv, astro-ph/0102200
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