VY Carinae, S Normae, and photometric luminosities for bright giants and supergiants of types G and K

Details VY Carinae, S Normae, and photometric luminosities for bright giants and supergiants of types G and K VY Carinae, S Normae, and photometric luminosities for bright giants and supergiants of types G and K

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..919e&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 15, 1980, p. 919-928.

Astronomy and Astrophysics

Astrophysics

33

Astronomical Photometry, Cepheid Variables, G Stars, Giant Stars, K Stars, Late Stars, Stellar Luminosity, Supergiant Stars, Calibrating, Early Stars, Interstellar Extinction, Star Distribution

Scientific paper

Observations in the modified Stromgren system of the Cepheids VY Carinae
and S Normae with their associated early-type stars are discussed. The
luminosities of the Cepheids, together with the bright giants R Puppis,
HR 2834, HR 4180, and HDE 269953 in the Large Magellanic Cloud (LMC),
are used for calibration of photometric luminosities.

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