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CO in Seyfert Galaxies

Published online by Cambridge University Press:  07 August 2017

Timothy M. Heckman
Timothy M. Heckman*
Affiliation:
Astronomy Program, University of Maryland, College Park, MD 20742, U.S.A.

Abstract

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We present data for Seyfert and normal galaxies in the Revised Shapley-Ames Catalog. The type 2 Seyferts are stronger CO and Far-IR emitters (by factors of 2–4) than either normal galaxies or type 1 Seyferts. The Seyfert CO line-widths correlate with both the 21cm HI and [OIII]5007 line-widths. Interferometer maps show that in many Seyferts the CO emission is strongly concentrated within radii of 100–1000pc of the nucleus. The implications of these results are briefly discussed.

Type
Part 7: Dust, Molecules, Infrared and MM Radiation
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 359 - 364
Copyright
Copyright © Kluwer 1989 

References

[1] Morris, M. and Rickard, L. J. 1982, Ann.Rev.Astr.Ap., 20, 517.CrossRefGoogle Scholar
[2] Norman, C. and Scoville, N. preprint.Google Scholar
[3] Sanders, R. and Bania, T. 1976, Ap.J., 204, 341.CrossRefGoogle Scholar
[4] van Breugel, W., Filippenko, A., Heckman, T., and Miley, G. 1985, Ap.J., 293, 83.CrossRefGoogle Scholar
[5] Terlevich, R. and Melnick, J. 1985, MNRAS, 213, 841.CrossRefGoogle Scholar
[6] Soifer, B., Houck, J., and Neugebauer, G. 1987, Ann.Rev.Astr.Ap., 25, 187.CrossRefGoogle Scholar
[7] Dame, T.M. etal. 1987, Ap.J., 322, 706.CrossRefGoogle Scholar
[8] Blitz, L., Bloemen, J., Hermsen, W., and Bania, T. 1985, Ap.J., 143, 267.Google Scholar
[9] Myers, S. T. and Scoville, N. 1987, Ap.J., 312, L39.CrossRefGoogle Scholar
[10] Lo, K.Y. etal. 1987, Ap. J. Lett., 317, L63.CrossRefGoogle Scholar
[11] Scoville, N. etal. 1986, Ap.J. Lett., 311, L47.CrossRefGoogle Scholar
[12] Becklin, E. and Wynn-Williams, G. 1987, in Star Formation in Galaxies, ed. Persson, C. (U.S. Govt. Printing Office), 753.Google Scholar
[13] Heckman, T., Miley, G., Butcher, H., and van Breugel, W. 1981, Ap.J., 247, 403.CrossRefGoogle Scholar
[14] Whittle, M. 1985, MNRAS, 213, 1.CrossRefGoogle Scholar
[15] Sanders, D. etal. 1986, Ap.J. Lett., 305, L45.CrossRefGoogle Scholar
[16] Kaneko, N. etal. 1988, preprint.Google Scholar
[17] Bloemen, J. etal. 1986, Astr. Ap., 154, 25.Google Scholar
[18] Miller, J. 1988, this volume.Google Scholar
[19] Simkin, S., Su, H., and Schwarz, M. 1980, Ap.J., 237, 404.CrossRefGoogle Scholar
[20] Schlosman, I., Frank, J., and Begelman, M. 1988, this volume.Google Scholar
[21] Krolik, J. and Vrtilek, J. 1984, Ap.J., 279, 521.CrossRefGoogle Scholar