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H2 Emission from External Galaxies

Published online by Cambridge University Press:  07 August 2017

Kimiaki Kawara
Kimiaki Kawara*
Affiliation:
National Astronomical Observatory Mitaka, Tokyo 181, Japan

Abstract

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2 μm spectroscopic observations by many authors have revealed significant rotation-vibrational H2 emission is widespread from starburst to bare nucleus galaxies. Near-IR H2 emission lines can arise from various excitation sources: UV radiation by hot stars, shock excitation by supernova remnants or AGN driven winds, and UV/X-ray radiation by an AGN. In this review recent data will be compared with such H2 excitation models.

Type
External Galaxies
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 103 - 107
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

Antonucci, R.R.J., and Miller, J.S. 1985, Ap.J., 297, 621.Google Scholar
Cambell, A. 1988, Ap.J., 335, 644.Google Scholar
Cecil, G., Bland, J., and Tully, R.B. 1990, Ap.J., 355, 70.Google Scholar
Drain, B.T., and Woods, D.T. 1990, Ap.J., 363, 464.Google Scholar
Fisher, J., Geballe, T.R., Smith, H.A., Simon, M., and Storey, J.W.V. 1987, Ap.J., 320, 667.CrossRefGoogle Scholar
Graham, J.R., Wright, G.S., and Longmore, A.J. 352, 172.Google Scholar
Joseph, R.D., Wright, G.S., Wade, R., Graham, J.R., Gatley, I., and Preswich, A.H. 1987, in Star Formation in Galaxies, ed. Lonsdale, C.J. (Washington, D.C.: US Government Printing Office), p421.Google Scholar
Kawara, K., Nishida, M., and Gregory, B. 1987, Ap.J. (Letters) 321, L35.CrossRefGoogle Scholar
Kawara, K., Nishida, M., and Gregory, B. 1989, Ap.J. (Letters) 342, L55.CrossRefGoogle Scholar
Kawara, K., Nishida, M., and Gregory, B. 1990, Ap.J. 352, 433.Google Scholar
Kawara, K., Nishida, M., and Taniguchi, Y. 1988, Ap.J. (Letters) 328, L41.Google Scholar
Koyama, K. 1989, in IAU symposium 134, Active Galactic Nuclei, ed. Osterbrock, D.E. and Miller, J.S. (Dordrecht: Kluwer), p. 167.Google Scholar
Krolik, J.H. and Begelman, M.C. 1986, Ap.J. (Letters) 308, L55.CrossRefGoogle Scholar
Krolik, J.H. and Lepp, S. 1989, Ap.J. 347, 179.Google Scholar
Lester, D.F., Harvey, P.M., and Carr, J. 1988, Ap.J., 329, 641.Google Scholar
Lepp, S., and McCray, R. 1983, Ap.J. 269, 560.Google Scholar
Moorwood, A.F.M., and Oliva, E. 1988, Astr. Ap., 203, 278.Google Scholar
Moorwood, A.F.M., and Oliva, E. 1990, Astr. Ap., 239, 78.Google Scholar
Mouri, H., Taniguchi, Y., Kawara, K., and Nishida, M. 1989, Ap.J. (Letters) 346, L73.CrossRefGoogle Scholar
Mouri, H., Kawara, K., Taniguchi, Y., and Nishida, M. 1990a, Ap.J. (Letters) 356, L39.Google Scholar
Mouri, H., Nishida, M., Taniguchi, Y., and Kawara, K. 1990b, Ap.J. 360, 55.Google Scholar
Mouri, H, and Taniguchi, Y. 1991, Ap.J. Private communication.Google Scholar
Rotacius, V., Krabbe, A., Cameron, M., Drapatz, S., Genzel, R., Sternberg, A., and Storey, J.W.V. 1991, Ap.J. (Letters) 370, L23.Google Scholar
Sternberg, A., and Dalgarno, A. 1989, Ap.J., 338, 197.Google Scholar
Tanaka, M., Hasegawa, T., and Gatley, I. 1991, Ap.J., 374, 516.Google Scholar
Veilleux, S., and Osterbrock, D.E. 1987, Ap.J. Suppl. 63, 295.Google Scholar