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Maximum Magnitude Vs. Rate of Decline for Novae of the LMC
Published online by Cambridge University Press: 12 April 2016
Abstract
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We derive the distance modulus of the Large Magellanic Cloud (LMC) by applying the new calibrated relationship between maximum magnitude and rate of decline (MMRD). The result, , is in close agreement with the most recent determinations based on RR Lyrae and Cepheids. We also discuss the properties of the MMRD of M31 and of the LMC.
- Type
- 1a. Basic Properties of Novae
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 71 - 72
- Copyright
- Copyright © Springer-Verlag 1990
References
Capaccioli, M., Della Valle, M., D’Onofrio, M., and Rosino, L.
1989a. Astron. Journal
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Capaccioli, M., Cappellaro, E., Della Valle, M., D’Onofrio, M., Rosino, L., and Turatto, M.
1989b. Astrophys. Journal, in press.Google Scholar
Capaccioli, M., Della Valle, M., D’Onofrio, M., and Rosino, L.
1989c. Astrophys. Journal submitted.Google Scholar
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