Hostname: page-component-84b7d79bbc-4hvwz Total loading time: 0 Render date: 2024-07-26T22:30:04.788Z Has data issue: false hasContentIssue false

RAPID STAR FORMATION IN GALACTIC NUCLEI

Published online by Cambridge University Press:  14 August 2015

G. H. Rieke*
Affiliation:
University of Arizona

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A large percentage of spiral galaxies are forming stars at a very high rate in their nuclei. There are indications that the process of star formation is modified significantly in these regions, compared with the solar neighborhood. The star formation may be fueled by interstellar material that is captured by the nucleus. Further work is needed to explore these possibilities and to establish the evolutionary connections among galactic nuclei, various types of which can be distinguished by their radically different infrared properties.

Type
Research Article
Copyright
Copyright © Reidel 1981 

References

Beck, S. C., Lacy, J. H., and Geballe, T. R.: 1979, Ap. J., 231, p.28.Google Scholar
Beck, S. C., Lacy, J. H., Baas, F., and Townes, C. H.: 1978, Ap. J., 226, p. 545.Google Scholar
Becklin, E. E., Gatley, I., Matthews, K., Neugebauer, G., Sellgren, K., Werner, M. W., and Wynn-Williams, C. G.: 1980, Ap. J., 236, p 441.Google Scholar
Faber, S. M., and French, H. B.: 1980, Ap. J., 235, p. 405.Google Scholar
Gillett, F. C., Kleinmann, D. E., Wright, E. L., and Capps, R. W.: 1975, Ap. J. (Letters), 198, p. L65.Google Scholar
Houck, J. R., Forrest, W. J., and McCarthy, J. F.: 1980, preprint.Google Scholar
Jones, T. W., Leung, C. M., Gould, R. J., and Stein, W. A.: 1977, Ap. J., 212, p. 52.Google Scholar
Kleinmann, D. E., and Low, F. J.: 1970, Ap. J. (Letters), 159, p. L165.Google Scholar
Larson, R. B., and Tinsley, B. M.: 1978, Ap. J., 219, p. 46.Google Scholar
Lebofsky, M. J., and Rieke, G. H.: 1979, Ap. J., 229, p. 111.Google Scholar
Oort, J. H.: 1977, Ann. Rev. Ast. Astrophys., 15, p. 295.Google Scholar
Pacholczyk, A. G., and Wisniewski, W. Z.: 1967, Ap. J., 147, p. 394.Google Scholar
Persson, S. E., Cohen, J. G., Sellgren, K., Mould, J., and Frogel, J. A.: 1980, Ap. J. (in press).Google Scholar
Rickard, L. J., Harvey, P. M., and Thronson, H. A.: 1980, paper presented at IAU Symposium 96.Google Scholar
Rieke, G. H., and Lebofsky, M. J.: 1978, Ap. J. (Letters), 220, p. L37.CrossRefGoogle Scholar
Rieke, G. H., and Low, F. J.: 1975, Ap. J., 197, p. 17.Google Scholar
Rieke, G. H., Lebofsky, M. J., Thompson, R. I., Low, F. J., and Tokunaga, A. T.: 1980, Ap. J., 238, p. 24.Google Scholar
Simon, M., Simon, T., and Joyce, R. R.: 1979, Ap. J., 227, p. 64.Google Scholar
Telesco, C. M., and Harper, D. A.: 1980, Ap. J. 235, p. 392.Google Scholar
Tonry, J., and Davis, M.: 1979, A. J., 84, p. 1511.Google Scholar
Willner, S. P., Soifer, B. T., Russell, R. W., Joyce, R. R., and Gillett, F. C.: 1977, Ap. J. (Letters), 217, p. L121.Google Scholar