Near-infrared surface photometry of NGC 253

Details Near-infrared surface photometry of NGC 253 Near-infrared surface photometry of NGC 253

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...259...97f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 259, no. 1, p. 97-100.

Astronomy and Astrophysics

Astronomy

24

Astronomical Photometry, Barred Galaxies, Galactic Structure, Infrared Astronomy, Field Of View, Near Infrared Radiation

Scientific paper

We present a large field-of-view H image of NGC 253 and discuss the galaxy's large scale infrared morphology and surface brightness profile. An iterative least-squares fit to the surface brightness profile gives the exponential disk and 'r exp 1/4' bulge parameters. We confirm the existence of a barred morphology not apparent at optical wavelengths and find that the derived disk scale length at H is slightly less than at B.

Affiliated with

Also associated with

No associations

Rating

Near-infrared surface photometry of NGC 253 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 Near-infrared surface photometry of NGC 253, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near-infrared surface photometry of NGC 253 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1199056