Hostname: page-component-7bb8b95d7b-nptnm Total loading time: 0 Render date: 2024-09-23T02:42:49.376Z Has data issue: false hasContentIssue false
  • English
  • Français

Dynamics of Early Type Galaxies

Published online by Cambridge University Press:  14 August 2015

F. Bertola  and
M. Capaccioli
F. Bertola
Affiliation:
Asiago Astrophysical Observatory, University of Padova, Italy
M. Capaccioli
Affiliation:
Asiago Astrophysical Observatory, University of Padova, Italy

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An attempt has been made to compute the angular momenta of the early type galaxies NGC 4697 and NGC 4762. Comparison with spiral galaxies indicates that there is a correlation between angular momentum per unit mass and morphological class.

Type
Part II/Flattened Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 373 - 375
Copyright
Copyright © Reidel 1975 

References

Bertola, F.: 1972, Atti XV Riunione SAIt, 199.Google Scholar
Bertola, F. and Capaccioli, M.: 1975, Astrophys. J., in press.Google Scholar
Capaccioli, M.: 1974, Atti Cel. V Cent. Coper., Univ. Padova, 109.Google Scholar
Houten, C. J. van: 1961, Bull. Astron. Inst. Neth. 16, 1.Google Scholar
Takase, B. and Kinoshita, H.: 1967, Publ. Astron. Soc. Japan 19, 131.Google Scholar