SIMBAD references

2015MNRAS.451..724W - Mon. Not. R. Astron. Soc., 451, 724-738 (2015/July-3)

Panchromatic Hubble Andromeda Treasury XIII: The Cepheid period-luminosity relation in M31.

WAGNER-KAISER R., SARAJEDINI A., DALCANTON J.J., WILLIAMS B.F. and DOLPHIN A.

Abstract (from CDS):

Using Hubble Space Telescope Advanced Camera for Surveys (HST/ACS) and Wide Field Camera 3 (WFC3) observations from the Panchromatic Hubble Andromeda Treasury (PHAT), we present new period-luminosity (P-L) relations for Cepheid variables in M31. Cepheids from several ground-based studies are identified in the PHAT photometry to derive new P-L and Wesenheit P-L relations in the near infrared and visual filters. We derive a distance modulus to M31 of 24.51±0.08 in the IR bands and 24.32±0.09 in the visual bands, including the first P-L relations in the F475W and F814W filters for M31. Our derived visual and IR distance moduli disagree at slightly more than a 1σ level. Differences in the P-L relations between ground-based and HST observations are investigated for a subset of Cepheids. We find a significant discrepancy between ground-based and HST P-L relations with the same Cepheids, suggesting adverse effects from photometric contamination in ground-based Cepheid observations. Additionally, a statistically significant radial trend in the P-L relation is found which does not appear to be explained by metallicity.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): stars: variables: Cepheids - galaxies: individual: - Local Group - distance scale

VizieR on-line data: <Available at CDS (J/MNRAS/451/724): table1.dat table2.dat>

Simbad objects: 183

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2019.10.23-11:01:57

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