Surface photometry of new nearby dwarf galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

accepted by A&A

Scientific paper

10.1051/0004-6361:20020006

We present CCD surface photometry of 16 nearby dwarf galaxies, many of which were only recently discovered. Our sample comprises both isolated galaxies and galaxies that are members of nearby galaxy groups. The observations were obtained in the Johnson B and V bands (and in some cases in Kron-Cousins I). We derive surface brightness profiles, total magnitudes, and integrated colors. For the 11 galaxies in our sample with distance estimates the absolute B magnitudes lie in the range of -10>Mb>-13. The central surface brightness ranges from 22.5 to 27.0 mag/sq.arcsec. Most of the dwarf galaxies show exponential light profiles with or without a central light depression. Integrated radial color gradients, where present, appear to indicate a more centrally concentrated younger population and a more extended older population.

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

Surface photometry of new nearby dwarf 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 Surface photometry of new nearby dwarf galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Surface photometry of new nearby dwarf galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-553653

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