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dc.contributor.authorWeilbacher, P.
dc.contributor.authorFritze, U.
dc.contributor.authorDuc, P.A.
dc.contributor.authorFricke, K.J.
dc.date.accessioned2007-10-18T10:00:40Z
dc.date.available2007-10-18T10:00:40Z
dc.date.issued2002-10-09
dc.identifier.citationWeilbacher , P , Fritze , U , Duc , P A & Fricke , K J 2002 , ' Large Velocity Gradients in the Tidal Tails of the Interacting Galaxy AM 1353-272 (The Dentist's Chair) ' , The Astrophysical Journal , vol. 579 , pp. L79-82 .
dc.identifier.issn1538-4357
dc.identifier.otherdspace: 2299/960
dc.identifier.urihttp://hdl.handle.net/2299/960
dc.description© 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
dc.description.abstractWe 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.en
dc.format.extent116107
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectPhysics
dc.titleLarge Velocity Gradients in the Tidal Tails of the Interacting Galaxy AM 1353-272 (The Dentist's Chair)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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