2000MNRAS.319....1T


Query : 2000MNRAS.319....1T

2000MNRAS.319....1T - Mon. Not. R. Astron. Soc., 319, 1-7 (2000/November-3)

Resonant capture, counter-rotating discs, and polar rings.

TREMAINE S. and YU Q.

Abstract (from CDS):

We suggest that polar rings and/or counter-rotating discs in flattened galaxies can be formed from stars captured at the Binney resonance, where the rate of precession of the angular momentum vector of a disc star equals the pattern speed of a triaxial halo. If the halo pattern speed is initially retrograde and slowly decays to zero, stars can be trapped as the Binney resonance sweeps past them, and levitated into polar orbits. If the halo pattern speed is initially retrograde and slowly changes to prograde, trapped stars can evolve from prograde to retrograde disc orbits.

Abstract Copyright: 2000, Royal Astronomical Society

Journal keyword(s): galaxies: formation - galaxies: general - galaxies: kinematics and dynamics

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 3593 GiG 11 14 36.9731893800 +12 49 05.497790664   11.8       ~ 376 2
2 NGC 4550 GiP 12 35 30.5913588048 +12 13 14.921166792 12.97 12.56 11.68     ~ 558 1
3 NGC 7217 LIN 22 07 52.3984675584 +31 21 33.632293572   12.94 11.92     ~ 511 0

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