A multiple galaxy collision in compact groups

It is shown that the dynamical paradox of the HCG 90, which is treated as an old, and at the same time, as a young system (White et al), may be solved assuming that it is a rotating system in which multiple collisions have occurred during Hubble time. In the frames of the same scenario a multiple co...

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Veröffentlicht in:	Astronomische Nachrichten 2003-11, Vol.324 (6), p.554-555
1. Verfasser:	Tovmassian, H.M.
Format:	Artikel
Sprache:	eng
Schlagworte:	galaxies: clusters: general galaxies: interactions galaxies: kinematics and dynamics
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description	It is shown that the dynamical paradox of the HCG 90, which is treated as an old, and at the same time, as a young system (White et al), may be solved assuming that it is a rotating system in which multiple collisions have occurred during Hubble time. In the frames of the same scenario a multiple collisions in SQ (HCG 92) are naturally explained. (© 2003 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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source	Wiley Online Library Journals Frontfile Complete
subjects	galaxies: clusters: general galaxies: interactions galaxies: kinematics and dynamics
title	A multiple galaxy collision in compact groups
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