Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...69..465k&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 69, no. 3, June 1987, p. 465-485.
Astronomy and Astrophysics
Astrophysics
39
Astronomical Catalogs, Electrophotometry, F Stars, G Stars, K Stars, Late Stars, M Stars, Spectral Energy Distribution, Stellar Luminosity, Astrometry, Radiant Flux Density, Southern Sky, Spectral Resolution, Stellar Evolution, Stellar Spectrophotometry
Scientific paper
Spectral energy distributions were photoelectrically measured from λ320 nm to λ860 nm with a resolution of 1 nm in equidistant steps of 1 nm for 60 bright southern and equatorial stars of intermediate and late spectral types for all luminosity classes. Flux curves for individual stars are plotted with a resolution of 1 nm and tabulated in steps of 5 nm. Typical internal mean errors of fluxes measured in different nights are less than 0m.02 in the spectral range from 400 nm to 860 nm, and rise to a maximum of about 0m.05 for wavelengths below 400 nm.
No associations
LandOfFree
Spectrophotometry of bright F-, G-, K- and M-type stars. I - Measurements of 60 southern and equatorial stars 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 Spectrophotometry of bright F-, G-, K- and M-type stars. I - Measurements of 60 southern and equatorial stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of bright F-, G-, K- and M-type stars. I - Measurements of 60 southern and equatorial stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1813529