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J/PAZh/28/653        Pulsation Modes of Cepheid                  (Sachkov, 2002)

Two Period-Radius Relations for Classical Cepheids: Determining the Pulsation Mode and the Distance Scale Sachkov M.E. <Pis'ma Astron. Zh. 28, 653 (2002)> =2002PAZh...28..653S =2002AstL...28..589S
ADC_Keywords: Stars, variable Abstract: A catalog of pulsation mode and radii for 64 classical Cepheids based on the 1995-2001 radial velocities observations with the correlation spectrometer. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file objects.dat 57 64 Objects positions table1.dat 44 13 First overtone Cepheid radii table2.dat 44 51 Fundamental mode Cepheid radii
Byte-by-byte Description of file: objects.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Star Name of the star system 12- 26 A15 --- OName Other star name 29- 30 I2 h RAh Right ascension (J2000) 32- 33 I2 min RAm Right ascension (J2000) 35- 41 F7.4 s RAs Right ascension (J2000) 43 A1 --- DE- [-+] Declination sign 44- 45 I2 deg DEd Declination (J2000) 47- 48 I2 arcmin DEm Declination (J2000) 50- 55 F6.3 arcsec DEs Declination (J2000)
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star name in GCVS 11- 16 F6.4 [d] logP1 Logarithm of first-overtone period 18- 20 I3 solRad Rad Cepheid Radius in solar units 22- 23 I2 solRad e_Rad Uncertainty in Rad 25- 29 F5.2 --- delPhi Phase shift 31- 34 F4.2 --- e_delPhi Uncertainty in delPhi 36- 39 F4.2 mag AmpV Amplitude in V-band 41- 44 F4.2 --- Mm Parameter of light curve in GCVS (G1)
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star name in GCVS 11- 16 F6.4 [d] logP0 Logarithm of fundamental-mode period 18- 20 I3 solRad Rad Cepheid Radius in solar units 22- 23 I2 solRad e_Rad Uncertainty in Rad 25- 29 F5.2 --- delPhi Phase shift 31- 34 F4.2 --- e_delPhi Uncertainty in delPhi 36- 39 F4.2 mag AmpV Amplitude in V-band 41- 44 F4.2 --- Mm Parameter of light curve in GCVS (G1)
Global Notes: Note (G1): Duration of brightness rise from minimum to maximum in fractions of the period.

(End) Mikhail Sachkov, Veta Avedisova (INASAN) 14-Nov-2002
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

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