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2009

Period-Luminosity Relation for Type II Cepheids

Matsunaga, Noriyuki, Feast, Michael W., Menzies, John W.

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We have estimated JHKs magnitudes corrected to mean intensity for LMC type II Cepheids found in the OGLE-III survey.

Period-luminosity relations (PLRs) are derived in JHKs as well as in a reddening-free VI parameter.
The BL Her stars (P<4d) and the W Vir stars (P=4 to 20d) are co-linear in these PLRs.
The slopes of the infrared relations agree with those found previously for type II Cepheids in globular clusters within the uncertainties.

Period-Luminosity Relation for Type II Cepheids · Around

Built on

Baade W., 1956, PASP, 68, 5
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Earlier work this paper cites.
Matsunaga N. et al., 2006, MNRAS, 370, 1979
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Lloyd Evans T., 1985, MNRAS, 217, 493
1985
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Bessell M. S., Brett J. M., 1988, PASP, 100, 1134
1988
Earlier work this paper cites.

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Then

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