Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy

Details Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pthph..64.1265m&link_type=abstract

Progress of Theoretical Physics, Vol. 64, No. 4, pp. 1265-1279

Physics

21

Scientific paper

The response of gas to an ovally deformed, rotating gravitational potential is investigated by following the time evolution of its motion using the Lin-Pringle quasi-particle technique. The results reveal that the gas responds to the presence of an oval distortion by forming a well-defined two-arm trailing spiral wave and elliptical rings rotating with the angular speed of the oval distortion.

Affiliated with

Also associated with

No associations

Rating

Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy 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 Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-950206