2010MNRAS.402..691D


Query : 2010MNRAS.402..691D

2010MNRAS.402..691D - Mon. Not. R. Astron. Soc., 402, 691-704 (2010/February-2)

Physical parameters of the Small Magellanic Cloud RR Lyrae stars and the distance scale.

DEB S. and SINGH H.P.

Abstract (from CDS):

We present a careful and detailed light curve analysis of RR Lyrae stars in the Small Magellanic Cloud (SMC) discovered by the Optical Gravitational Lensing Experiment (OGLE) project. Out of 536 single-mode RR Lyrae stars selected from the data base, we have investigated the physical properties of 335 `normal-looking' RRab stars and 17 RRc stars that have good quality photometric light curves. We have also been able to estimate the distance modulus of the cloud which is in good agreement with those determined from other independent methods. The Fourier decomposition method has been used to study the basic properties of these variables. Accurate Fourier decomposition parameters of 536 RR Lyrae stars in the OGLE-II data base are computed. Empirical relations between the Fourier parameters and some physical parameters of these variables have been used to estimate the physical parameters for the stars from the Fourier analysis. Further, the Fourier decomposition of the light curves of the SMC RR Lyrae stars yields their mean physical parameters as and MV = 0.78±0.02 for 335 RRab variables and and MV = 0.76±0.05 for 17 RRc stars. Using the absolute magnitude together with the mean magnitude, intensity-weighted mean magnitude and the phase-weighted mean magnitude of the RR Lyrae stars, the mean distance modulus to the SMC is estimated to be 18.86±0.01, 18.83±0.01 and 18.84±0.01 mag, respectively, from the RRab stars. From the RRc stars, the corresponding distance modulus values are found to be 18.92±0.04, 18.89±0.04 and 18.89±0.04 mag, respectively. Since the Fourier analysis is a very powerful tool for the study of the physical properties of the RR Lyrae stars, we emphasize the importance of exploring the reliability of the calculation of Fourier parameters together with the uncertainty estimates keeping in view the large collections of photometric light curves that will become available from variable star projects of the future.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): methods: data analysis - astronomical data bases: miscellaneous - stars: fundamental parameters - stars: variables: other - Magellanic Clouds

VizieR on-line data: <Available at CDS (J/MNRAS/402/691): table1.dat table2.dat table5.dat table6.dat>

Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 NGC 121 GlC 00 26 49.0 -71 32 10   11.2 11.24     ~ 286 0
2 M 31 G 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 11377 1
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 9859 1
4 NGC 361 OpC 01 02 12.83 -71 36 16.2 12.86 12.43 11.77   10.70 ~ 95 0
5 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 5997 1
6 NGC 1851 GlC 05 14 06.76 -40 02 47.6           ~ 1289 0
7 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 15467 1
8 M 68 GlC 12 39 27.98 -26 44 38.6   10.26 7.96     ~ 913 0
9 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2326 0
10 NGC 5466 GlC 14 05 27.29 +28 32 04.0   10.5 9.70     ~ 754 0
11 IC 4499 GlC 15 00 18.57 -82 12 49.6     8.56     ~ 320 0
12 M 5 GlC 15 18 33.22 +02 04 51.7   7.34 5.95     ~ 1829 0

    Equat.    Gal    SGal    Ecl

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2021.07.30-17:27:40

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