New Distances to the Magellanic Clouds

Details New Distances to the Magellanic Clouds New Distances to the Magellanic Clouds

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cto..conf..223v&link_type=abstract

Cepheids: Theory and Observations, Proceedings of IAU Colloquium No. 82, held 29 May - 1 June, 1984 in Toronto, Canada. Edited

Physics

2

Scientific paper

The mean phase magnitudes at the IV waveband (1.05 micron) of thirteen Cepheids in the SMC and the LMC and nine Cepheids in groups and clusters in the Galaxy, are used in conjunction with periods, to construct P-L(IV) relations in these galaxies. The slopes and the dispersions of the relations are nearly the same. The authors derives a distance modulus of 19.11±0.07 for the SMC and 18.82±0.07 for the LMC.

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