Comparison of the Bahcall / Soneira Galaxy Model with Observations

Details Comparison of the Bahcall / Soneira Galaxy Model with Observations Comparison of the Bahcall / Soneira Galaxy Model with Observations

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..209b&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Computer Science

2

Scientific paper

Modern data on the distribution of stellar colors and on the number of stars as a function of apparent magnitude in five directions in the Galaxy are analyzed. Observational studies by various authors are analyzed. All of the data are described well by a two-component model with an exponential disk and a de Vaucouleurs spheroid. The fat-disk model proposed by Gilmore and Reid does not fit the results of Kron for SA57 and of Koo and Kron for SA68.

Affiliated with

Also associated with

No associations

Rating

Comparison of the Bahcall / Soneira Galaxy Model with Observations 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 Comparison of the Bahcall / Soneira Galaxy Model with Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of the Bahcall / Soneira Galaxy Model with Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1508831