Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-09-15
Astron.J.121:140-147,2001
Astronomy and Astrophysics
Astrophysics
19 pages, 4 figures, AJ, accepted
Scientific paper
10.1086/318027
We measure the frequency of bulk gas-stellar counterrotation in a sample of 67 galaxies drawn from the Nearby Field Galaxy Survey, a broadly representative survey of the local galaxy population down to M_B-15. We detect 4 counterrotators among 17 E/S0's with extended gas emission (24% +8 -6). In contrast, we find no clear examples of bulk counterrotation among 38 Sa-Sbc spirals, although one Sa does show peculiar gas kinematics. This result implies that, at 95% confidence, no more than 8% of Sa-Sbc spirals are bulk counterrotators. Among types Sc and later, we identify only one possible counterrotator, a Magellanic irregular. We use these results together with the physical properties of the counterrotators to constrain possible origins for this phenomenon.
Fabricant Dan G.
Kannappan Sheila J.
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