Classification of Galaxies by Their Radial Profiles: Unbarred Early Types

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

We classify 46 broad band surface-brightness profiles in the visible from a sample of nearby early-type unbarred galaxies imaged at the ING (La Palma) and in the SDSS. A key result is that the fraction of these galaxies showing truncations in their outer disks is relatively small (of order 10%). The largest single category of galaxies show what tet{erwin05} have termed ``Type III'' profiles, which have an exponential inner disk, and also an exponential outer disk but with a shallower slope. They show no sign of truncations out to beyond at least five scale-lengths. The second most frequent category is that of tet{free70} ``Type I'' disks, which show a single exponential slope out to the radial limits of detection, with no sign of any truncation. Together, Types I and III account for over 75% of the galaxies in our sample. This is part of an ongoing program to use galaxy surface-brightness profiles to test models of galaxy formation.

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

Classification of Galaxies by Their Radial Profiles: Unbarred Early Types 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 Classification of Galaxies by Their Radial Profiles: Unbarred Early Types, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classification of Galaxies by Their Radial Profiles: Unbarred Early Types will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1244363

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