Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723

Details Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723 Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....107..631a&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 107, no. 2, p. 631-633

Astronomy and Astrophysics

Astronomy

5

Astronomical Photography, Calibrating, Globular Clusters, Photoelectricity, Stellar Spectrophotometry, Ubv Spectra, Charge Coupled Devices, Stellar Color, Stellar Magnitude

Scientific paper

UBVRI photoelectric sequences for the galactic globular clusters IC 4499 and NGC 6723 are herewith presented. Both of them include fields suitable for charge coupled devices (CCD) coverage. The number of stars and the range of magnitude and colors are: IC 4499, eight stars with 12.5 less than V less than 15.3; 0.7 less than B - V less than 1.7; NGC 6723, seventeen stars with 10.4 less than V less than 15.6; 0.4 less than B - V less than 1.6. The stars were measured an average of eight times on at least four different nights. One stars of IC 4499 and twelve in NGC 6723 are in common with previous works.

Affiliated with

Also associated with

No associations

Rating

Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723 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 Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photoelectric UBVRI sequences in the galactic globular clusters IC 4499 and NGC 6723 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1013582