A period luminosity relation for supergiant red variables in the Large Magellanic Cloud

Details A period luminosity relation for supergiant red variables in the Large Magellanic Cloud A period luminosity relation for supergiant red variables in the Large Magellanic Cloud

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..377f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 377-380.

Astronomy and Astrophysics

Astronomy

28

Magellanic Clouds, Periodic Variations, Red Giant Stars, Stellar Luminosity, Supergiant Stars, Variable Stars, Bolometers, Infrared Photometry, Photometry, Stellar Magnitude

Scientific paper

Infrared photometry for 24 red supergiant variables in the LMC is used
to derive bolometric magnitudes. The existence of a period-luminosity
relation for these stars is demonstrated and compared with theory.

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