The Cepheid Distance Scale: a New Application for Infrared Photometry.

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Scientific paper

Broadband photometry has been obtained at J (1.25 (mu)m), H (1.65 (mu)m), and K (2.2 (mu)m) for a sample of Cepheids in the Large Magellanic Cloud, Small Magellanic Cloud, and in galactic clusters/associations. We have measured arbitrary-phase magnitudes for 43 LMC, 28 SMC, and 8 galactic Cepheids, enabling us to calibrate the J, H, and K Period-Luminosity (P-L) relations and obtain distances to the LMC and SMC based on J, H, K photometry. These distances are:. (UNFORMATTED TABLE FOLLOWS). LMC: (m-M)(,o) = 18('('m))42 + 0.67 * E(B-V),. SMC: (m-M)(,o) = 18('('m))94 + 0.67 * E(B-V). (TABLE ENDS). We illustrate, by comparison of the optical and infrared P-L relations, that the infrared is markedly less affected by extinction, temperature, duplicity, and metallicity, the net result being that P-L relations based on arbitrary -phase infrared magnitudes are competitive with those based on mean optical magnitudes. A comparison of the V, H, and (B-V) data for the LMC and SMC confirms the existence of a second parameter, believed to be temperature, causing correlated changes in V, H, and (B-V) and giving rise to the Period-Luminosity -Colour (P-L-C) relation. A comparison of the V and H data, after removing their log P and (B-V) dependences, reveals the presence of yet a third parameter. This parameter causes correlated changes, of approximately equal magnitude, in V and H. Differential reddening, combined with temperature, can qualitatively explain this effect but the slope of the relation appears anomalous.

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