Galaxy mass distributions for some extreme orbital-speed Profiles

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5 pages, 5 figures, PDF

Scientific paper

Extreme speed profiles, that are impossible to anayze correctly using the usual methods, are shown to be easily handled using the methods developed previously by Nicholson (astro-ph/0006330). These profiles are constant orbital speeds with sharp and smooth ramps at the origin, and constant angular velocity with speeds increasing linearly to the galaxy rim. Also an example using measured data for a real galaxy is shown for NGC 3198. A new format is presented to show results in dimensionless form, that includes a way to show SMD results so they are easily compared. Based on repeated trials for accuracy, the rod representing the mass of a fundamental segment is now placed at 0.575*dr at the center ring of a galaxy.

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

Galaxy mass distributions for some extreme orbital-speed Profiles 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 Galaxy mass distributions for some extreme orbital-speed Profiles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galaxy mass distributions for some extreme orbital-speed Profiles will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-2416

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