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Dark Galaxies: How about this one?

Published online by Cambridge University Press:  01 June 2007

Christian Struve ,
Gyula I.G. Józsa ,
Franz Kenn ,
Uli Klein  and
Gianfranco Gentile
Christian Struve
Affiliation:
Netherlands Foundation for Research in Astronomy, P.O. Box 2, 7990 AA Dwingeloo, The Netherlands; email: struve@astron.nl Kapteyn Institute, Univ. of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands
Gyula I.G. Józsa
Affiliation:
Argelander-Institut für Astronomie, Univ. of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
Franz Kenn
Affiliation:
Argelander-Institut für Astronomie, Univ. of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
Uli Klein
Affiliation:
Argelander-Institut für Astronomie, Univ. of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
Gianfranco Gentile
Affiliation:
Univ. of New Mexico, Dept. of Physics and Astronomy, 800 Yale Blvd NE, Albuquerque, NM 87131, USA.
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Abstract

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We report on the (serendipitous) detection and analysis of an extremely massive HI cloud without an obvious stellar counterpart nearby the relatively isolated giant spiral galaxy NGC 1030 and present first results of this dark galaxy candidate.

Keywords

Galaxies: kinematics and dynamicsgalaxies: ISMgalaxies: interactionsgalaxies: structuregalaxies: individual: NGC 1030
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S244: Dark Galaxies and Lost Baryons , June 2007 , pp. 387 - 388
Copyright
Copyright © International Astronomical Union 2008

References

Bournaud, F. & Duc, P.-A. 2006, A&A 456, 481Google Scholar
Józsa, G., Kenn, F., Klein, U., Oosterloo, T. 2007, A&A 468, 731Google Scholar
Struve, C., Józsa, G., Kenn, F., Klein, U., Pizella, A. & Salucci, P. 2007, NewAR 51, 120CrossRefGoogle Scholar