C. -C. Ngeow, M. Marconi, I. Musella, M. Cignoni, M. Marengo, S. Kanbur
The mid-infrared period-luminosity (P-L) relation for Cepheids will be
important in the JWST era, as it holds the promise of deriving the Hubble
constant within 2% accuracy. We present the synthetic P-L and period-color
(P-C) relations, derived from a series of stellar pulsation models with varying
helium and metallicity abundance, in the Spitzer IRAC bands. Selected synthetic
P-L and P-C relations were compared to the empirical relations derived from
Galactic and Large Magellanic Cloud Cepheids. We also present the empirical P-L
relations based on the latest distance measurements using infrared surface
brightness techniques.
View original:
http://arxiv.org/abs/1111.2100
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