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The Gas Content in Disk Galaxies through Centimetric Radio, Infrared and Optical Windows

Published online by Cambridge University Press:  03 August 2017

G. Gavazzi
G. Gavazzi*
Affiliation:
Osservatorio Astronomico di Brera via Brera, 28, Milano, Italy

Abstract

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I wish to discuss two basic questions:

1) what do we know from the observations about the relationships between the physical conditions of the Interstellar medium (ISM) in disk galaxies and their past and present star formation rate, heating of dust and acceleration of relativistic cosmic rays ?

2) are the above relations and mechanisms sensitive to the intergalactic environment in rich clusters of galaxies?

I will discuss these questions by reviewing three topics:

a) gas content versus star formation

b) FIR emission versus star formation

c) radio continuum emission versus star formation and by discussing weather and how these topics are related to the environment.

Type
XII- Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 403 - 410
Copyright
Copyright © Kluwer 1991 

References

Bicay, M. and Giovanelli, R., 1987, Ap.J. 321, 645 CrossRefGoogle Scholar
Burstein, D., Condon, J., and Yin, Q., 1987, Ap.J., 315, L99 CrossRefGoogle Scholar
Devereux, N., and Young, J., 1990, Ap.J. 350, L25 CrossRefGoogle Scholar
Dickey, J., and Gavazzi, G., 1990, Submitted to Ap.J. Google Scholar
Donas, J., Buat, V., Millard, B., Laget, M., 1990, A.A, in press Google Scholar
Fanti, C., Fanti, R., Feretti, L., Ficarra, A., Gioia, I., Giovannini, G., Gregorini, L., Mantovani, F., Marano, B., Padrielli, L., Parma, P., Tomasi, P., and Vettolani, G., 1982, A.A., 105, 200 Google Scholar
Gavazzi, G., and Perola, C., 1980, A.A., 84, 228 Google Scholar
Gavazzi, G., and Jaffe, W., 1986, Ap.J., 310, 53 CrossRefGoogle Scholar
Gavazzi, G., Cocito, A., and Vettolani, G., 1986, Ap.J., 305, L15 CrossRefGoogle Scholar
Gavazzi, G., 1988, in: “The MInnesota Lectures on Clusters of Galaxies and Large-Scale Structure”, Ed.Dickey, J., PASP, p.115 Google Scholar
Gavazzi, G., 1989, Ap.J., 346, 59 CrossRefGoogle Scholar
Giovanelli, R., and Haynes, M., 1985, Ap.J., 292, 404 CrossRefGoogle Scholar
Guideroni, B., 1987, A.A., 172, 27 Google Scholar
Gunn, J., and Gott, J., 1972, Ap.J., 176, 1 CrossRefGoogle Scholar
Haynes, M., Giovanelli, R., and Chincarini, G., 1984, Ann.Rew.Astron.Astrophys, 22, 445 CrossRefGoogle Scholar
Hummel, E., 1981, A.A., 93, 93 Google Scholar
Kenney, J., and Young, J., 1989, Ap.J., 344, 171 CrossRefGoogle Scholar
Kenney, J., 1989, Proc. II Wyoming conference: “The ISM in Galaxies”. ed. Thronson, H. and Shull, M. Google Scholar
Kennicutt, R., 1983, A.A., 120, 219 Google Scholar
Kennicutt, R., 1989, Ap.J., 344, 685 CrossRefGoogle Scholar
Klein, U., 1882, A.A., 15, 42 Google Scholar
Kotanyi, C., 1980, A.A. Suppl., 41, 421 Google Scholar
Lonsdale-Perrson, C., Helou, G., 1987, Ap.J., 314, 513 CrossRefGoogle Scholar
Nulsen, P., 1982, M.N.R.A.S., 198, 1007 CrossRefGoogle Scholar
Perola, C., and Valentjin, E., 1979, A.A., 73, 54 Google Scholar
Perola, C., Tarenghi, M., and Valentyin, E., 1980, A.A., 85, 245 Google Scholar
Schmidt, M., 1959, Ap.J., 129, 243 CrossRefGoogle Scholar
Seiden, P., 1983, Ap.J., 266, 555 CrossRefGoogle Scholar
Stark, A., Knapp, G., Bally, J., Wilson, R., Penzias, A., and Rowe, H., 1986, Ap.J., 310, 660 CrossRefGoogle Scholar
Sullivan, W., Bothun, G., Bates, B., and Schommer, R., 1981, A.J., 86, 919 CrossRefGoogle Scholar
Young, J., 1989, Proc. II Wyoming conference:“The ISM in Galaxies”. ed. Thronson, H. and Shull, M. Google Scholar
Zwicky, F., et al, 1961-1968: “Catalogue of Galaxies and Clusters of Galaxies”. Pasadena: California Institute of Technology Press.Google Scholar