J/other/RMxAA/54.15         Variable stars in NGC 6934            (Yepez+, 2018)

The variable star population in the globular cluster NGC 6934. Yepez M.A., Arellano Ferro A., Muneer S., Giridhar S. <Rev. Mex. Astron. Astrofis., 54, 15-36 (2018)> =2018RMxAA..54...15Y 2018RMxAA..54...15Y (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, globular ; Stars, variable ; Photometry, CCD Keywords: globular clusters: individual: NGC 6934 - stars: variables: RR Lyrae - stars: variables: SX Phe Abstract: We report an analysis of new V and I CCD time-series photometry of the globular cluster NGC 6934. Through the Fourier decomposition of the RR Lyrae light curves, the mean values of [Fe/H] and the distance of the cluster were estimated, we found; [Fe/H]UVES=-1.48±0.14 and d=16.03±0.42kpc, and [Fe/H]UVES=-1.43±0.11 and d=15.91±0.39kpc, from the calibrations of RRab and RRc stars respectively. Independent distance estimations from SX Phe and SR stars are also discussed. Individual absolute magnitudes, radii and masses are also reported for RR Lyrae stars. We found 12 new variables: 4 RRab, 3 SX Phe, 2 W Virginis (CW) and 3 semi-regular (SR). The inter-mode or "either-or" region in the instability strip is shared by the RRab and RRc stars. This characteristic, observed only in some OoI clusters and never seen in an OoII, is discussed in terms of mass distribution in the ZAHB. Description: V and I time-series photometry for all confirmed variables in NGC 6934. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 87 104 General data of confirmed variables in NGC 6934 table6.dat 92 31237 VI photometry of 34 RR Lyrae, 14 SX Phe, 1 SR -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- VName Variable name, VNN 4 A1 --- n_VName [a] a for newly found in this work 6- 11 A6 --- Type Variable type 13- 18 F6.3 mag ?=- Intensity weighted V magnitude 20- 25 F6.3 mag ?=- Intensity weighted I magnitude 27- 31 F5.3 mag AV ?=- V amplitude 33- 37 F5.3 mag AI ?=- I amplitude 38 A1 --- u_AI Uncertainty flag on AI 39 A1 --- l_PKOS01 [~] Limit flag on PKOS01 40- 48 F9.6 d PKOS01 ?=- Period Kaluzni et al. (2001AJ....121.1533K 2001AJ....121.1533K) 50- 58 F9.4 d E0 ?=- Epoch (HJD-2450000) 60- 67 F8.6 d Per ?=- Period present work 69- 70 I2 h RAh ?=- Right ascension (J2000) 72- 73 I2 min RAm ?=- Right ascension (J2000) 75- 78 F4.1 s RAs ?=- Right ascension (J2000) 79 A1 --- DE- Declination sign (J2000) 80- 81 I2 deg DEd ?=- Declination (J2000) 83- 84 I2 arcmin DEm ?=- Declintaion (J2000) 86- 87 I2 arcsec DEs ?=- Declination (J2000) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 A3 --- VName Variable name, VNN 7 A1 --- Filter [VI] Observation filter 10- 22 F13.5 d HJD Heliocentric Julian date 25- 30 F6.3 mag magst Standard magnitude 33- 38 F6.3 mag maginst Instrumental magnitude 41- 45 F5.3 mag e_maginst ?=- Error on the magnitude 49- 57 F9.3 s-1 Fref Reference flux (in ADU/s) 60- 65 F6.3 s-1 e_Fref Error on the reference flux (in ADU/s) 68- 76 F9.3 s-1 DFlux ?=- Differential flux (in ADU/s) 79- 84 F6.3 s-1 e_DFlux ?=- Error on the differential flux (in ADU/s) 87- 92 F6.4 --- p Photometric scale factor -------------------------------------------------------------------------------- Acknowledgements: Armando Arellano Ferro, armando(at)astro.unam.mx
(End) A. Arelano Ferro [IA-UNAM, Mexico], P. Vannier [CDS] 17-May-2018
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line