Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-01-05
Mon.Not.Roy.Astron.Soc.376:809-819,2007
Astronomy and Astrophysics
Astrophysics
11 pages, 9 figures, accepted for publication in MNRAS
Scientific paper
10.1111/j.1365-2966.2007.11477.x
We study the effect of spiral arm passages on the evolution of star clusters on planar and circular orbits around the centres of galaxies. Individual passages with different relative velocity (V_drift) and arm width are studied using N-body simulations. When the ratio of the time it takes the cluster to cross the density wave to the crossing time of stars in the cluster is much smaller than one, the energy gain of stars can be predicted accurately in the impulsive approximation. When this ratio is much larger than one, the cluster is heated adiabatically and the net effect of heating is largely damped. For a given duration of the perturbation, this ratio is smaller for stars in the outer parts of the cluster compared to stars in the inner part. The cluster energy gain due to perturbations of various duration as obtained from our N-body simulations is in good agreement with theoretical predictions taking into account the effect of adiabatic damping. Perturbations by the broad stellar component of the spiral arms on a cluster are in the adiabatic regime and, therefore, hardly contribute to the energy gain and mass loss of the cluster. We consider the effect of crossings through the high density shocked gas in the spiral arms, which result in a more impulsive compression of the cluster. The time scale of disruption is shortest at ~0.8-0.9 R_CR since there V_drift is low. This location can be applicable to the solar neighbourhood. In addition, the four-armed spiral pattern of the Milky Way makes spiral arms contribute more to the disruption of clusters than in a similar but two-armed galaxy. Still, the disruption time due to spiral arm perturbations there is about an order of magnitude higher than what is observed for the solar neighbourhood.[ABRIDGED]
Athanassoula Evangelia
Gieles Mark
Portegies Zwart Simon. F.
No associations
LandOfFree
The effect of spiral arm passages on the evolution of stellar clusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The effect of spiral arm passages on the evolution of stellar clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The effect of spiral arm passages on the evolution of stellar clusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-15812