Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-18T21:59:20.676Z Has data issue: false hasContentIssue false
  • English
  • Français

The Plume Phenomenon in Barred Spirals

Published online by Cambridge University Press:  25 April 2016

R. Buta
R. Buta*
Affiliation:
Mount Stromlo and Siding Spring Observatories, Research School of Physical Sciences, Australian National University
Get access Rights & Permissions [Opens in a new window]

Extract

Barred spirals are well-known to include several ‘distinct components’ or morphological structures in the light distribution (Sandage 1961; de Vaucouleurs 1959; Kormendy 1979). In addition to the bar, spheroid, and disk components, one often observes ring-like enhancements at discrete relative positions within the disk. These inner rings (r), outer rings (R), and nuclear rings (nr) have been the subject of recent, fairly intensive observational (Buta 1984a; Kormendy J979; de Vaucouleurs and Buta 1980a,b; Athanassoula et al. 1982) and theoretical (Schwarz 1979,1981,1984a,b,c; Simkin, Su, and Schwarz 1980) research, and it now seems well-established that most rings are linked to dynamical resonances with the bar.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 472 - 478
Copyright
Copyright © Astronomical Society of Australia 1984

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Athanassoula, E., Bosma, A., Creze, M., and Schwarz, M. P., Astron. Astrophys. 107, 101 (1982).Google Scholar
Buta, R., Ph.D. Thesis, The University of Texas at Austin (1984a).Google Scholar
Buta, R., paper in preparation (1984b).Google Scholar
Buta, R., paper in preparation (1984c).Google Scholar
Contopoulos, G., in Photometry, Kinematics, and Dynamics of Galaxies, ed. Evans, D. S. (Department of Astronomy, University of Texas at Austin), p. 425 (1979).Google Scholar
Contopoulos, G. and Papayannopoulos, T., Astron. Astrophys. 92, 33 (1980).Google Scholar
de Vaucouleurs, G., Handbuch der Physik 53, 275 (1959).Google Scholar
de Vaucouleurs, G. and Buta, R., Astron. J. 85, 637 (1980a).Google Scholar
de Vaucouleurs, G. and Buta, R., Astrophys. J. Suppl. 44, 451 (1980b).Google Scholar
de Vaucouleurs, G., de Vaucouleurs, G., and Corwin, H. G., Second Reference Catalogue of Bright Galaxies (Austin: University of Texas Press) (1976). (RC2)Google Scholar
Hohl, F., Astrophys, J., 168, 343 (1971).Google Scholar
Kormendy, J., Astrophys. J. 227, 714 (1979).Google Scholar
Kormendy, J., in Morphology and Dynamics of Galaxies, (Geneva Observatory), p. 115 (1982).Google Scholar
Lynden-Bell, D. and Kalnajs, A. J., Mon. Not. R. Astron. Soc. 157, 1 (1972).Google Scholar
Sandage, A., The Hubble Atlas of Galaxies (Carnegie Institution of Washington Publ. No. 618) (1961).Google Scholar
Sandage, A. and Tammann, G. A., A Revised Shapley-Ames Catalogue of Bright Galaxies (Carnegie Institution of Washington Publication No. 635). (1981).Google Scholar
Schwarz, M. P., PhD Thesis, Australian National University (1979).Google Scholar
Schwarz, M. P., Astrophys. J. 247, 77 (1981).Google Scholar
Schwarz, M. P., Astron. Astrophys. 133, 222 (1984a).Google Scholar
Schwarz, M. P., Monthly Notices R. A. S. 209, 93 (1984b).CrossRefGoogle Scholar
Schwarz, M. P., Proc. Astron. Soc. Aust. 5, (1984c).Google Scholar
Shu, F. H., Milione, V., and Roberts, W. W., Astrophys J. 183, 819 (1973).Google Scholar
Simkin, S. M., Su, H. J., and Schwarz, M. P., Astrophys. J. 237, 404 (1980).Google Scholar