UBV photometry of stars whose positions are accurately known. VII

Details UBV photometry of stars whose positions are accurately known. VII UBV photometry of stars whose positions are accurately known. VII

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..100..591o&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 100, no. 3, p. 591, 592.

Astronomy and Astrophysics

Astronomy

1

Faint Objects, Sky Surveys (Astronomy), Stellar Color, Stellar Magnitude, Astronomical Photometry, Interstellar Extinction, Stellar Luminosity

Scientific paper

Attention is given to UBV photometry for about 100 equatorial and southern stars of the faint extension of the FK5 catalog which previously lacked accurate V photometry. The observations were performed with the 60-cm Cassegrain telescope of the Royal Swedish Academy of Sciences at La Palma, Canary Islands, during February-March and August-September 1992. Extinction coefficients were derived, separately for every night, for the V magnitude as well as for the colors.

Affiliated with

Also associated with

No associations

Rating

UBV photometry of stars whose positions are accurately known. VII 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 UBV photometry of stars whose positions are accurately known. VII, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV photometry of stars whose positions are accurately known. VII will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1559060