Inertial Effects From Companion Galaxies Driving Warps in Disk Galaxies

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

While most disk galaxies are observed to be warped, the mechanisms for the warping are not well understood. We explore warping caused by gravitational perturbations created by the passage of a distant galaxy (the 'intruder'). We propose that the intruder's effect on the disk galaxy can be explained in terms of pseudoforces that occur while the two galaxies interact. We carry out N-Body simulations with plausible interaction parameters that give significant warps having amplitudes comparable to those observed in some disk galaxies. The interacting galaxies have typical separations of 150-200 kpc and the intruder galaxy is moving at angles of 30, 45, 60, and 90 degrees relative to the plane of the disk galaxy. For each simulation we obtained integral-like shapes for the disk galaxy. (Simulations with other separations and interaction angles generated the other classifications of warps, called `feeble’ and `irregular.') Further observations of galaxies with these signature integral-shaped warps, located in the vicinity of massive neighbors, would support the existence of this mechanism. (Funding was provided by the Maine Space Grant Consortium and Boston University.)

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Inertial Effects From Companion Galaxies Driving Warps in Disk Galaxies 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 Inertial Effects From Companion Galaxies Driving Warps in Disk Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Inertial Effects From Companion Galaxies Driving Warps in Disk Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-965436

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.