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Some Remarks on Observational Problems for Disk-Galaxy Evolution

Published online by Cambridge University Press:  03 August 2017

M. Sanromà ,
E. Salvador-Solé  and
J.M. Solanes
M. Sanromà
Affiliation:
Dpt. de Física de l'Atmòsfera, Astronomia i Astrofísica. Univ. de Barcelona. Av. Diagonal 647. 08028 Barcelona. Spain
E. Salvador-Solé
Affiliation:
Dpt. de Física de l'Atmòsfera, Astronomia i Astrofísica. Univ. de Barcelona. Av. Diagonal 647. 08028 Barcelona. Spain
J.M. Solanes
Affiliation:
Dpt. de Física de l'Atmòsfera, Astronomia i Astrofísica. Univ. de Barcelona. Av. Diagonal 647. 08028 Barcelona. Spain

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Observational objections against an important role of evolution in morphological differentiation of disk - galaxies (Burnstein 1979, Dressier 1980b, Kent 1985) are summarized together with the results of their det ailed analysis (Salvador-Solé et al. 1987a and 1987b):

  1. i) Morphological segregation is independent on cluster characteristics.

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 581
Copyright
Copyright © Reidel 1988 

References

Burstein, D. 1979. Ap.J. 234, 435 CrossRefGoogle Scholar
Dressler, A. 1980a. Ap.J. Suppl. 42, 565 CrossRefGoogle Scholar
Dressler, A. 1980b. Ap.J. 236, 351 CrossRefGoogle Scholar
Kent, S.M. 1985. Ap.J. Suppl. 59, 115 CrossRefGoogle Scholar
Salvador-Solé, E., Sanromà, M., Rdez. Jordana, J.J. 1987a. Ap.J. (submitted) Google Scholar
Salvador-Solé, E., Sanromà, M., Solanes, J.M. 1987b. Ap.J. Lett. (submitted) Google Scholar