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HI Absorption Detection in the Perseus Cooling Flow

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Cooling Flows in Clusters and Galaxies

Part of the book series: NATO ASI Series ((ASIC,volume 229))

Abstract

With the Westerbork Synthesis Radio Telescope (WSRT) we detect HI absorption at 5250 km/s in front of the nucleus of NGC 1275, with an optical depth of .003 and a dispersion of 205 km/s. We do not detect HI associated with the 30″ halo in absorption or emission.

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References

  • Crane, P.C., van de Hulst, J.M., Haschick A.D., 1982 in Extragalactic Radio Sources, IAU Symposium 97, Reidel, Dordrecht, p. 307

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  • Jaffe, W. 1987, Astron & Astrophys 171, 378

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  • O’Dea, C.P., Baum, S.A. 1987, Astron. J. in press

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Author information

Authors and Affiliations

  1. Sterrewacht Leiden, P.O. Box 9513, 2300 RA, Leiden, NL

    W. J. Jaffe

  2. Radiosterrewacht te Dwingeloo, Oudehoogeveensedijk 4, 7991 PD, Dwingeloo, NL

    A. G. de Bruyn

  3. Kapteijn Laboratorium, P.O. Box 800, 9747 AE, Groningen, NL

    D. Sijbreng

Authors
  1. W. J. Jaffe
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  2. A. G. de Bruyn
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  3. D. Sijbreng
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Editor information

Editors and Affiliations

  1. Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 OHA, UK

    A. C. Fabian

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© 1988 Kluwer Academic Publishers

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Jaffe, W.J., de Bruyn, A.G., Sijbreng, D. (1988). HI Absorption Detection in the Perseus Cooling Flow. In: Fabian, A.C. (eds) Cooling Flows in Clusters and Galaxies. NATO ASI Series, vol 229. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2953-1_16

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  • DOI: https://doi.org/10.1007/978-94-009-2953-1_16

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7828-3

  • Online ISBN: 978-94-009-2953-1

  • eBook Packages: Springer Book Archive

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