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Bulge Morphology of Non-Interacting Starburst Galaxies

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Dynamics and Interactions of Galaxies

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Abstract

If a starburst occurs in the circumnuclear zone of a non-interacting galaxy, a consequence is to sweep out the interstellar gas in a galactic wind (J.E. Beckman [l], C. Muñoz-Tuñón and J.E. Beckman [2]). Repeated starbursts can occur if there is a mechanism for refuelling the nuclear zone. Following Zaritsky and Lo [3], we are exploring the suggestion that departures from bulge axisymmetry can lead to this type of inflow.

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References

  1. J. E. Beckman: Mass Outflows from Stars and Galactic Nuclei in L. Bianchi and R. Gilmozze eds., Kluwer, p. 385 (1988)

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  2. C. Muñoz-Tuñón, J. E. Beckman: Ap. Sp. Sci. 147, 173 (1988)

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  3. D. Zaritsky and K. Y. Lo: Ap. J., 303, 66 (1986)

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Author information

Authors and Affiliations

  1. Instituto de Astrofísica de Canarias, Spain

    A. M. Varela, J. E. Beckman, J. Cepa, C. Muñoz-Tuñon, M. Prieto & J. M. Vilchez

  2. Observatorio del Roque de los Muchachos, La Palma, Spain

    J. Cepa & J. M. Vilchez

  3. Departamento de Física Fundamental, Universidad de la Laguna, Spain

    C. Muñoz-Tuñon

Authors
  1. A. M. Varela
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  2. J. E. Beckman
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  3. J. Cepa
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  4. C. Muñoz-Tuñon
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  5. M. Prieto
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  6. J. M. Vilchez
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Editor information

Editors and Affiliations

  1. Astronomisches Rechen-Institut, Mönchhofstrasse 12-14, D-6900, Heidelberg 1, Fed. Rep. of Germany

    Roland Wielen

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© 1990 Springer-Verlag Berlin Heidelberg

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Varela, A.M., Beckman, J.E., Cepa, J., Muñoz-Tuñon, C., Prieto, M., Vilchez, J.M. (1990). Bulge Morphology of Non-Interacting Starburst Galaxies. In: Wielen, R. (eds) Dynamics and Interactions of Galaxies. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-75273-5_43

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  • DOI: https://doi.org/10.1007/978-3-642-75273-5_43

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-75275-9

  • Online ISBN: 978-3-642-75273-5

  • eBook Packages: Springer Book Archive

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