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Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation pp 99–100Cite as

Molecular Gas in Nuclei of the Seyfert Galaxies NGC3227 and NGC1068

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Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

Abstract.

New subarcsecond data on NGC 3227 and NGC 1068 obtained with the Plateau de Bure millimeter interferometry indicate large enclosed masses and the possibility of warped molecular gas disks.

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Authors and Affiliations

  1. California Institute of Technology, Pasadena, CA 91125, USA

    Eva Schinnerer

  2. Max-Planck-Institut für extraterrestrische Physik, 85740, Garching, Germany

    Andreas Eckart & Linda Tacconi

Authors
  1. Eva Schinnerer
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  2. Andreas Eckart
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  3. Linda Tacconi
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Editor information

Lex Kaper Edward P. J. van den Heuvel Patrick A. Woudt

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Schinnerer, E., Eckart, A., Tacconi, L. Molecular Gas in Nuclei of the Seyfert Galaxies NGC3227 and NGC1068. In: Kaper, L., Heuvel, E.P.J.v.d., Woudt, P.A. (eds) Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10720995_16

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  • DOI: https://doi.org/10.1007/10720995_16

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-41581-7

  • Online ISBN: 978-3-540-44562-3

  • eBook Packages: Springer Book Archive

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