Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793

Details Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793 Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jass....3...53k&link_type=abstract

Journal of Astronomy and Space Science, vol. 3, no. 1, p. 53-66.

Astronomy and Astrophysics

Astronomy

Scientific paper

Isophotes and surface brightness distribution were obtained for the late type normal spiral galaxy NGC 7793 (morphological type SA(s)d) which is one of the Sculptor group. The calculated total luminosity BT is obtained as 9.44 and the corrected face on magnitude B degT is 9.10. The revised distance to this galaxy ¡â = 3.1 Mpc (de Vaucouleurs and Davoust 1980) is used for calculating the absolute magnitude M¢ªT = -18.36. From the isophotes, the position angle to the major axis is 101 deg, the mean axial ratio is q= b/a = 0.65, and the inclination is i = 50deg. The concentric indices C21 = 1.69 and C32 = 1.50 are well agreed to the average value of Sd type galaxies.

Affiliated with

Also associated with

No associations

Rating

Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793 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 Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical Parameters of Late Type Spiral Galaxies-II Surface Brightness Distribution of NGC7793 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1833415