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Large Velocity Gradients in the Tidal Tails of the Interacting Galaxy AM 1353–272 ("The Dentist's Chair")*

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Published 2001 October 9 © 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Peter M. Weilbacher et al 2002 ApJ 579 L79 DOI 10.1086/345318

1538-4357/579/2/L79

Abstract

We present Very Large Telescope observations of the interacting system AM 1353-272. Using the FORS2 instrument, we studied the kinematics of the ionized gas along its prominent tidal tails and discovered strikingly large velocity gradients associated with seven luminous tidal knots. These kinematical structures cannot be caused by streaming motion and most likely do not result from projection effects. More probably, instabilities in the tidal tails have led to the formation of kinematically decoupled objects that could be the progenitors of self-gravitating tidal dwarf galaxies.

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Footnotes

  • Based on observations collected at the European Southern Observatory, La Silla, Chile (ESO 67.B-0049).

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10.1086/345318