Abstract
Observed supernovae rates in Sb and Sc galaxies, and a recent re-examination of the mean gas density in these galactic types, implies that if the ‘clumpiness’ of gas in the disks of Sb and Sc galaxies is similar, the gas density isnot the primary factor in determining the overall present stellar birthrate.
Similar content being viewed by others
References
Einasto, J.: 1972,Astron. Astrophys. 11, 195.
Field, G. B. and Saslaw, W. C.: 1965,Astrophys. J. 142, 568.
Field, G. B. and Hutchins, J.: 1968,Astrophys. J. 153, 737.
Gordon, K. J.: 1971,Astrophys. J. 169, 235.
Hartwick, F. D. H.: 1971,Astrophys. J. 163, 431.
Ilovaisky, S. H. and Lequeux, J.: 1972,Astron. Astrophys. 18, 169.
Kellman S. A. and Black, D. C.: 1973,Astrophys. J. 184, 753.
Larson, R. B.: 1969,Monthly Notices Roy. Astron. 145, 271.
Quirk, W. J.: 1972,Astrophys. J. 176, L9.
Quirk, W. J. and Tinsley, B. M.: 1973,Astrophys. J. 179, 69.
Sanduleak, N.: 1969,Astron. J. 74, 47.
Schmidt, M.: 1959,Astrophys. J. 129, 243.
Tammann, G.: 1970,Astron. Astrophys. 8, 458.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Black, D.C., Kellman, S.A. Is the present stellar birthrate really determined by gas density?. Astrophys Space Sci 26, 107–109 (1974). https://doi.org/10.1007/BF00642624
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00642624