Photometry of F-K type bright giants and supergiants. I - Intermediate band and H-Beta observations

Details Photometry of F-K type bright giants and supergiants. I - Intermediate band and H-Beta observations Photometry of F-K type bright giants and supergiants. I - Intermediate band and H-Beta observations

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....103.1381e&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 103, April 1992, p. 1381-1388.

Astronomy and Astrophysics

Astronomy

5

Astronomical Photometry, F Stars, H Beta Line, K Stars, Supergiant Stars, Spectral Line Width, Stellar Luminosity, Stellar Spectra

Scientific paper

Over 1500 observations of 560 bright giants and supergiants of types F-K are presented and compared to the observations by Gray and Olsen (1991). The present results include intermediate-band which is slightly different from the Stromgren data by Gray and Olsen due to a different width for the v filter. A systematic difference in m(1) - M(1) with decreasing temperature is noted in the two H-Beta data sets, and the correlations are defined.

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