J/AJ/129/433  Abundances and equivalent widths of 14 Cepheids  (Kovtyukh+, 2005)

Phase-dependent variation of the fundamental parameters of cepheids. II. Periods longer than 10 days. Kovtyukh V.V., Andrievsky S.M., Belik S.I., Luck R.E. <Astron. J., 129, 433-453 (2005)> =2005AJ....129..433K 2005AJ....129..433K
ADC_Keywords: Stars, variable ; Abundances ; Equivalent widths Keywords: Cepheids - stars: abundances Abstract: We present the results of a detailed multiphase spectroscopic analysis of 14 classical Cepheids with pulsation periods longer than 10 days. For each star, we have derived phased values of effective temperature, surface gravity, microturbulent velocity, and elemental abundances. We show that the elemental abundance results for these Cepheids are consistent for all pulsational phases. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table5.dat 64 186 Observing log table6.dat 55 122016 Line equivalent widths table7.dat 33 6138 Per-phase abundances -------------------------------------------------------------------------------- See also: J/A+A/381/32 : Galactic Cepheid abundances (Andrievsky+, 2002) J/A+A/392/491 : Galactic abundance gradient. III. (Andrievsky+, 2002) J/A+A/413/159 : Galactic abundance gradient. V. (Andrievsky+, 2004) J/AJ/113/1073 : Abundances in Cepheid Variables (Fry+ 1997) Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Name Cepheid name 8- 18 F11.8 d Per Period 20- 26 A7 --- Tel Telescope 28- 37 A10 "YYYY-MM-DD" ObsDate Date of the observation (YYYY-MM-DD) 39- 49 F11.3 d JD Julian Date of observation 51- 55 F5.3 --- Phase Phase of Cepheid 57- 60 I4 s ExpTime ? Exposure time 62- 64 I3 --- S/N Mean signal-to-noise ratio -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Name Cepheid name 8- 13 A6 --- Ion Ion 15- 22 F8.3 0.1nm lambda Wavelength 24- 27 F4.1 --- Z Atomic number 28- 29 A2 --- --- [00] 31- 36 F6.3 eV EP Lower excitation potential 38- 44 F7.3 --- loggf Oscillator strength 46- 50 F5.3 --- Phase Phase in Cepheid 52- 55 I4 pm EW ? Line equivalent width at Phase -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 F4.1 --- Z Atomic number (1) 6- 11 A6 --- Name Cepheid name 14- 18 F5.3 --- Phase Phase 20- 24 F5.2 [Sun] Abund ?=-9.99 Abundance of element Z 26- 29 F4.2 [Sun] e_Abund ?=0 Standard deviation of Abundance 31- 33 I3 --- o_Abund ?=0 Number of lines for the species -------------------------------------------------------------------------------- Note (1): The first decimal is 0 for the neutral atom, and 1 for the ionized atom (e.g. 26.0 = Fe I and 26.1 = Fe II). -------------------------------------------------------------------------------- History: From electronic version of the journal References: Luck & Andrievsky, Paper I 2004AJ....128..343L 2004AJ....128..343L
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 25-Aug-2005
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