Abstract
High surface brightness galaxies are also galaxies with high star-forming activity. About a half of them omit, on the average, twice as much energy in the IR than in the blue. The rates of star formation are 10–30 times higher than those in normal galaxies. On average 100–300 solar masses gas are converted into stars every year and 10–30 are massive stars.
References
Arakelian, M. A.: 1975,Contr. Bjurakan Obs. 47, 3.
Catalogued Galaxies and Quasars detected in the IRAS Survey: 1985.
De Jong, T., Clegg, P., Soifer, B., Rowan-Robinson, M., and Habing, H.: 1984,Astrophys. J. 278, L67.
Desert, F. X.: 1986, in F. Israel (ed.),Light on Dark Matter, D. Reidel Publ. Co., Dordrecht, Holland.
Fasano, G.: 1985,Astron. Astrophys., Suppl. 60, 285.
Helou, G.: 1986,Astrophys. J. 311, L33.
Houck, J., Soifer, B., Neugebauer, G., Beichmann, C., and Auman, H.: 1984,Astrophys. J. 278, L63.
Nilson, P.: 1973,Uppsala General Catalogue of Galaxies, Uppsala.
Petrov, G. T.: 1986,Astrophys. Space Sci. 124, 407.
Petrov, G. T.: 1988, (in press).
Soifer, B., Houck, J., and Neugebauer, G.: 1987,Ann. Rev. Astron. Astrophys. 25, 187.
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Petrov, G.T. Star burst activity in high surface brightness galaxies. Astrophys Space Sci 151, 169–175 (1989). https://doi.org/10.1007/BF00643639
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DOI: https://doi.org/10.1007/BF00643639