Disk-to-halo Mass Ratio Evaluations Based on the Numerical Models of Collisionless Disks

Details Disk-to-halo Mass Ratio Evaluations Based on the Numerical Models of Collisionless Disks Disk-to-halo Mass Ratio Evaluations Based on the Numerical Models of Collisionless Disks

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006assl..337..307z&link_type=toc

Astrophysical Disks. Edited by Alexei M. Fridman, Institute of Astronomy, Moscow, Russia; Mikhail Ya. Marov, Keldysh Institute o

Astronomy and Astrophysics

Astronomy

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