RGU photometry in a field of the galactic bulge

Details RGU photometry in a field of the galactic bulge RGU photometry in a field of the galactic bulge

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...51..533s&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 51, Mar. 1983, p. 533-539. Research supported by the Swiss National Science

Astronomy and Astrophysics

Astrophysics

4

Astronomical Photometry, Galactic Bulge, Galactic Structure, Halos, Ultraviolet Photometry, Visual Photometry, Distance, Dwarf Stars, Giant Stars, Late Stars, Space Density, Subdwarf Stars

Scientific paper

Photometric parallaxes of 1800 stars in a field centred on l = 0°, b = 29° have been determined using complete RGU photometry down to mG = 18m.7. The density functions for the dwarfs and photometric subdwarfs are presented as well as the one for the late type giants. The observed density function of the late type giants, which is complete up to 19 kpc, is compatible with the density function predicted from the standard two component model of Bahcall and Soneira (1980) assuming a distance to the galactic centre of 8 kpc.

Affiliated with

Also associated with

No associations

Rating

RGU photometry in a field of the galactic bulge 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 RGU photometry in a field of the galactic bulge, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RGU photometry in a field of the galactic bulge will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1464971