Kinematic study of the ring galaxy Arp 10.

Details Kinematic study of the ring galaxy Arp 10. Kinematic study of the ring galaxy Arp 10.

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap.....41..106r&link_type=abstract

Astrophysics, Volume 41, Issue 2, pp.106-111

Astronomy and Astrophysics

Astrophysics

1

Peculiar Galaxies: Kinematics, Interacting Galaxies: Kinematics, Interacting Galaxies: Ring Galaxies

Scientific paper

The results of a kinematic study of the peculiar galaxy Arp 10 carried out on the 6- m telescope of the Special Astrophysical Observatory, Russian Academy of Sciences, are given. The galaxy exhibits a complex velocity field, a departure of integral characteristics from the Tully — Fisher relation, a low mass-to-luminosity ratio, and an enhanced rate of star formation. The hypothesis that the observed features of Arp 10 were formed in the accretion of a companion onto a gas-rich spiral galaxy is discussed.

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