Structure of the Spiral Galaxy NGC 300

Details Structure of the Spiral Galaxy NGC 300 Structure of the Spiral Galaxy NGC 300

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jass....9...11r&link_type=abstract

Journal of Astronomy and Space Sciences, vol.9, no.1, p.11-29.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

In 1963, Toomre built up classes of mass models for the highly flattened galaxies which have free parameters n, an and Cn. In order to keep the universal dimension, we adopt parameters bn(Cn2 = an2n+2bn2/(n-1)!) instead of Cn. Series of the normalized Toomre's mass models (G = Vmax = Rmax = 1, n =1 to 7) are derived and the normalized parameters an and bn to an(=anrmax) and bn(=bnVmax/rmax), we can get the generalization of Toomre's mass model.

Affiliated with

Also associated with

No associations

Rating

Structure of the Spiral Galaxy NGC 300 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 Structure of the Spiral Galaxy NGC 300, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of the Spiral Galaxy NGC 300 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1205812