Distance of the Large Magellanic Cloud through the maximum magnitude versus rate of decline relation for novae

Details Distance of the Large Magellanic Cloud through the maximum magnitude versus rate of decline relation for novae Distance of the Large Magellanic Cloud through the maximum magnitude versus rate of decline relation for novae

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...360...63c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 360, Sept. 1, 1990, p. 63-67.

Mathematics

Logic

45

Astrometry, Magellanic Clouds, Novae, Andromeda Galaxy, Cepheid Variables, Light Curve

Scientific paper

The magnitudes at maximum and the rates of decline of the LMC novae are reviewed. The distance modulus of the LMC is derived at 18.70 + 0.20 or - 0.25 by applying the newly calibrated maximum magnitude versus rate of decline (MMRD) relationship. The result is in close agreement with determinations based on Cepheids. The MMRD properties in galaxies of different morphological types are compared.

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