J/MNRAS/446/4008    RT Aur and SZ tau UBV light curves       (Evans+, 2015)

Observations of Cepheids with the MOST satellite: contrast between pulsation modes. Evans N.R., Szabo R., Derekas A., Szabados L., Cameron C., Matthews J.M., Sasselov D., Kuschnig R., Rowe J.F., Guenther D.B., Moffat A.F.J., Rucinski S.M., Weiss W.W. <Mon. Not. R. Astron. Soc., 446, 4008-4018 (2015)> =2015MNRAS.446.4008E 2015MNRAS.446.4008E (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Photometry, UBV Keywords: techniques: photometric - stars: individual: RT Aur - stars: individual: SZ Tau - stars: variables: Cepheids Abstract: The quantity and quality of satellite photometric data strings is revealing details in Cepheid variation at very low levels. Specifically, we observed a Cepheid pulsating in the fundamental mode and one pulsating in the first overtone with the Canadian MOST (Microvariability and Oscillations of Stars) satellite. The 3.7-d period fundamental mode pulsator (RT Aur) has a light curve that repeats precisely, and can be modelled by a Fourier series very accurately. The overtone pulsator (SZ Tau, 3.1d period) on the other hand shows light-curve variation from cycle to cycle which we characterize by the variations in the Fourier parameters. We present arguments that we are seeing instability in the pulsation cycle of the overtone pulsator, and that this is also a characteristic of the O-C curves of overtone pulsators. On the other hand, deviations from cycle to cycle as a function of pulsation phase follow a similar pattern in both stars, increasing after minimum radius. In summary, pulsation in the overtone pulsator is less stable than that of the fundamental mode pulsator at both long and short time-scales. Description: The MOST satellite is a photometric satellite fully described in Walker et al. (2003PASP..115.1023W 2003PASP..115.1023W), with the first science presented in Matthews et al. (2004Natur.430...51M 2004Natur.430...51M). For SZ Tau, observations were obtained in 2012 November (JD 2456238 - JD 2456257) resulting in a continuous data set covering 19d with a cadence of 1-min. For RT Aur, the observations were carried out in 2012 December 2012 (JD 2456278 - JD 2456300). For this target, the 22d-long observations were interleaved with another target, resulting in gaps in the light curve. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 06 28 34.09 +30 29 34.9 RT Aur = HD 45412 04 37 14.78 +18 32 34.9 SZ Tau = HD 29260 ----------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 29 89 O-C values of RT Aurigae table5.dat 29 38 O-C values of SZ Tauri table6.dat 28 36 New UBV photometric data of SZ Tau refs.dat 96 21 References -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.4 d HJD Heliocentric Julian date (HJD-2400000) 12- 16 I5 --- E Epoch of the determination in cycles 18- 24 F7.4 d O-C Observed minus computed time 26 I1 --- W Weigth 28- 29 I2 --- Ref Reference for the data -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 F10.4 d HJD Heliocentric Julian date (HJD-2400000) 12- 16 F5.3 mag Vmag V magnitude 18- 22 F5.3 mag B-V B-V colour index 24- 28 F5.3 mag U-B ?=- U-B colour index -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Ref Reference number 4- 22 A19 --- BibCode BibCode 24- 44 A21 --- Aut Author's name 46- 96 A51 --- Com Comments -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 23-Jul-2015
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