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J/other/BSAO/38.152    Effective temperatures of CP stars (Glagolevskij 1994)

A new list of effective temperatures of chemically peculiar stars. II. Glagolevskij Yu.V. <Bull. Special Astrophys. Obs., 38, 152 (1994)> =1994BSAO...38..152G (SIMBAD/NED BibCode)
ADC_Keywords: Stars, peculiar ; Effective temperatures ; Photometry Abstract: A new list is presented of effective temperatures estimated for about 700 chemically peculiar stars from the photometric parameters, calibrated with the temperatures determined by Shallis Blackwell (Blackwell et al., 1980A&A....82..249B) method from the total flux of the energy emitted by the stars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 21 26 Dependence of parameters Q and X upon the effective temperatures table2.dat 76 671 Effective temperatures of chemically peculiar stars
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 5 I5 K Teff Effective temperature (1) 7- 12 F6.3 --- Q Q parameter (2) 14- 17 F4.2 --- X X parameter (2)
Note (1): Construction of these dependences is based on the papers of Megessier (1988A&AS...72..551M), Stepien and Dominiczak (1989A&A...219..197S), Lamers (1981ApJ...245..593L), Shallis et al. (1985MNRAS.213..307S) and Glushneva (1987AZh....64..601G). Note (2): Q parameter: reddening free index. See Johnson et al., 1953ApJ...117..313J X parameter: parameter of multicolour photometry
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 6 I6 --- HD ? HD number 7 A1 --- m_HD Multiplicity index on HD 9- 19 A11 --- BD ? BD or CPD number 21- 25 I5 K Teff(Q) ? Effective temperature from parameter Q 26 A1 --- u_Teff(Q) Uncertainty flag on Teff(Q) 28- 32 I5 K Teff(X) ? Effective temperature from parameter X of multicolour photometry 34- 38 I5 K Teff(M) ? Effective temperature from total flux in Megessier (1988A&AS...72..551M) 39 A1 --- n_Teff(M) [+*] Note on Teff(M) (1) 41- 45 I5 K Teff(SD) ? Effective temperature from Stepien and Dominiczak (1989A&A...219..197S) 48- 52 I5 K Teff(L) ? Effective temperature from Lanz (1985A&A...144..191L) 54- 58 I5 K Teff(Sh) ? Effective temperature from Shallis et al. (1985MNRAS.213..307S)x; 60- 64 I5 K Teff(A) ? Effective temperature from Adelman's serie of papers 65 A1 --- u_Teff(A) Uncertainty flag on Teff(A) 67- 71 I5 K Teff0 Average temperatures from Teff(Q), Teff(X), Teff(M), Teff(SD), Teff(L) and Teff(Sh) 72 A1 --- u_Teff0 Uncertainty flag on Teff0 73 A1 --- n_Teff0 [m*] Note (2) 74 I1 % DeltaT ? Deviation of individual T from the average values T
Note (1): +: temperatures averaged from T(2100), T(u-b) and T(B2-G) *: temperature estimated for CP stars T<10500K from (B2-G) photometry Note (2): Temperature marked by * estimated for CP stars T<10500K from (B2-G) photometry, the metallic-line stars (marked "m") have own calibration (B2-V1)-Te (see the text and paper by Hauck & North, 1993A&A...269..403H).
History: Prepared via OCR at CDS. References: Glagolevskij, 1990, In: Hot chemically peculiar and magnetic stars, Potsdam-Babelsberg, 43 (Paper I.)
(End) James Marcout, Patricia Bauer [CDS] 25-Aug-1998
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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