Abstract
We present surface photometry and stellar kinematics of NGC 4431, a barred dwarf galaxy in the Virgo Cluster undergoing a tidal interaction with one of its neighbors, NGC 4436. We measured its bar pattern speed using the Tremaine-Weinberg method and derived the ratio of the corotation radius, D L, to the bar semimajor axis, aB. We found D L/aB = 0.6-0.4+1.2 at 99% confidence level. Albeit with large uncertainty, the probability that the bar ends close to its corotation radius (i.e., 1.0 ≤ DLaB ≤ 1.4) is about twice as likely as that the bar is much shorter than the corotation radius (i.e., DL/aB > 1.4).
| Original language | English |
|---|---|
| Pages (from-to) | L121-L124 |
| Journal | Astrophysical Journal |
| Volume | 659 |
| Issue number | 2 II |
| DOIs | |
| Publication status | Published - 20 Apr 2007 |
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