Stellar and ionized gas kinematics in NGC 2855 (Corsini+, 2002)

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Galaxies: Rotation, Radial Velocities

Scientific paper

We present major and minor-axis kinematics of stars and ionized gas as well as narrow and broad-band surface photometry of the Sa spiral NGC 2855. In the nuclear regions of this unbarred and apparently undisturbed spiral galaxy the gas is rotating perpendicularly to the galaxy disk. We suggest that this kinematically-decoupled component is the signature of an acquisition process in the history of this galaxy. (2 data files).

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

Stellar and ionized gas kinematics in NGC 2855 (Corsini+, 2002) 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 Stellar and ionized gas kinematics in NGC 2855 (Corsini+, 2002), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar and ionized gas kinematics in NGC 2855 (Corsini+, 2002) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1188271

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