V/118 Catalog of eclipsing binaries parameters (Perevozkina+, 1999)
Catalogue of orbital elements, masses and luminosities of detached main sequence
type eclipsing binaries with known elements of photometric orbit and unknown
spectroscopic elements.
Perevozkina E.L., Svechnikov M.A.
<Catalogue of orbital elements, masses and luminosities of eclipsing binaries
with detached main sequence components and some results of statistic
processing. 1999, ed. I.I. Bondarenko, Ekaterinburg, Ural. Univers.>
ADC_Keywords: Binaries, orbits; Combined data ; Binaries, eclipsing ;
Stars, masses ; Stars, diameters
Abstract:
This catalogue contains information about 44 binaries with known
photometric orbit elements and unknown spectroscopic one.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
catalog.dat 159 44 Catalog
notes.dat 79 68 Individual notes
refs.dat 103 48 References
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Byte-by-byte Description of file: catalog.dat
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Bytes Format Units Label Explanations
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1- 2 I2 --- Seq [1/44] Number of the system
3 A1 --- n_Seq [*] note detailed in notes.dat file
5- 13 A9 --- Name Name of eclipsing binary system
16- 26 F11.8 d Per Orbital period
27 A1 --- n_Per '*' marks period variability
30- 47 A18 --- SpType Spectral classes and luminosity classes
of components
49- 54 F6.3 --- q Mass ratio M2/M1
55 A1 --- u_q Uncertainty flag on q
57- 61 F5.2 solRad A Orbital semi-major axis
64- 68 F5.2 solMass M1 Mass of the first component
70- 74 F5.2 solMass M2 Mass of the second component
75 A1 --- u_M2 Uncertainty flag on M2
77- 80 F4.2 solRad R1 Radius of the first component
83- 86 F4.2 solRad R2 Radius of the second component
87 A1 --- u_R2 Uncertainty flag on R2
90- 95 F6.3 mag Mbol1 Absolute Bolometric magnitude of comp. 1 (1)
98-103 F6.3 mag Mbol2 Absolute Bolometric magnitude of comp. 2 (1)
106-111 F6.4 --- r1 Relative radius of the primary component
(mean radius of components) in units of A
113-118 F6.4 --- r2 Relative radius of the secondary component
(mean radius of components) in units of A
121-125 F5.3 --- L1 Relative brightness of the primary
component (in units of L1+L2=1)
126 A1 --- u_L1 Uncertainty flag on L1
127-128 A2 --- lambda Effective spectral band used for observation
129 A1 --- n_lambda [#] '#' marks L1 when observations were made
in wavelengths near to V or B.
132-138 F7.3 --- J1/J2 Ratio of surface brightnesses of primary
component to secondary one
140-141 A2 --- lambdaJ Effective spectral band used for observations
144-148 F5.2 deg i Orbit plane inclination
149 A1 --- u_i Uncertainty flag on i
150 A1 --- l_W Limit flag on W
151 A1 --- W Weight defined the reliability of photometric
and absolute elements determination in
ten-point scale (2)
154-158 A5 --- r_Seq References, detailed in refs.dat file
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Note (1): Mbol were computed using their geometrical characteristics,
spectral classes and luminosity classes as put above. Effective
temperatures of stars were taken in Popper D., 1980ARA&A..18..115P 1980ARA&A..18..115P.
Note (2): Criteria assumed as a basis for weight evaluation are
investigated more in detail in Svechnikov M.A., 1969, Catalogue
of orbital elements, masses ant luminosities of compact binaries,
Uchen. zap. Izd. Ural. un-ta. 88. Ser. astronom., 5.
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Byte-by-byte Description of file: notes.dat
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Bytes Format Units Label Explanations
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1- 2 I2 --- Seq Sequential number
4- 79 A76 --- Note Text of the note
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Byte-by-byte Description of file: refs.dat
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Bytes Format Units Label Explanations
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1- 2 I2 --- Ref Reference number
4- 22 A19 --- BibCode BibCode
24- 48 A25 --- Aut Author's name
49-102 A54 --- Com Comments
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(End) Rozaliya Saitgaraeva(Moscow University] Veta Avedisova(INASAN) 24-May-2004