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The external origin of the gas in S0 galaxies

Publications: Contribution to journalArticlePeer Reviewed

Abstract

In this Letter we present three new cases of S0 galaxies, namely NGC 2768, NGC 4379, and IC 4889, out of a sample of 15, in which the gas is counterrotating or strongly kinematically decoupled with respect to the stellar body of the galaxy. Assuming gas infall with randomly oriented angular momentum, this result implies that in 40% of the galaxies in our sample, the ionized gas is of external origin. However, several pieces of evidence suggest that the acquisition of external gas in S0 galaxies can be even more general.
Original languageEnglish
JournalThe Astrophysical Journal: an international review of astronomy and astronomical physics
Volume401
Issue number2 PART 2
Publication statusPublished - 1993

Austrian Fields of Science 2012

  • 103003 Astronomy

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