Summary
A new method to derive the kinetic energies associated to rotational and random motions from the observed rotation curve and velocity dispersion profile of elleptical galaxies is presented. The method also provides an estimate of the virial mass and of the total angular momentum.
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Presented at the Second Italian-Korean Meeting on Relativistic Astrophysics held at the University of Rome and in Limone Piemonte in July 1989.
To speed up publication, proofs were not sent to the authors and were supervised by the Scientific Committee.
OAC-FORMEZ fellow.
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Busarello, G., Longo, G. & Feoli, A. A new method to compute kinetic energy, virial mass and angular momentum of elliptical galaxies. Nuovo Cim B 105, 1069–1077 (1990). https://doi.org/10.1007/BF02741577
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DOI: https://doi.org/10.1007/BF02741577