On the rotational velocities of interacting galaxies

Details On the rotational velocities of interacting galaxies On the rotational velocities of interacting galaxies

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.211..155r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 211, no. 1, p. 155-160

Astronomy and Astrophysics

Astrophysics

2

Binary Stars, Interacting Galaxies, Spiral Galaxies, Mass To Light Ratios, Maxima, Rotation, Velocity

Scientific paper

A sample of members of close-binary interacting galaxies with the known values of the maximum rotational velocities are considered. It is found that the spiral galaxies in interacting systems tend to have lower rotational velocities and smaller mass to luminosity ratios than their counterparts in the field. The Tully-Fisher relationship may be different for interacting and field galaxies.

Affiliated with

Also associated with

No associations

Rating

On the rotational velocities of interacting 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 On the rotational velocities of interacting galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the rotational velocities of interacting galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-865276