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J/PAZh/29/571         X-ray fluxes of radio pulsars              (Malov, 2003)

On the mechanism of X-ray emission from radio pulsars. Malov I.F. <Pis'ma Astron. Zh. 29, 571 (2004)> =2003PAZh...29..571M =2003AstL...29..502M
ADC_Keywords: Radio sources ; Pulsars ; X-ray sources ; Magnetic fields Keywords: pulsars, neutron stars and black holes: X-ray sources Abstract: We discuss the correlations between the luminosities of radio pulsars in various frequency ranges and the magnetic fields of the light cylinder. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table.dat 30 155 Pulsars with η≥24
See also: J/AZh/71/762 : Radio luminosities of 232 pulsars (Malov+, 1994) Byte-by-byte Description of file: table.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Sequential number 4 A1 --- n_Seq [*] *: pulsar with measured X-ray fluxes (Possenti et al., 2002A&A...387..993P) 6- 15 A10 --- PSR PSR designation 18 A1 --- l_logeta Limit flag on logeta 19- 22 F4.2 [---] logeta eta value (1) 24 A1 --- l_logF Limit flag on logF 25- 30 F6.2 [mW/m2] logF X-ray flux in the 2-10keV band (1)
Note (1): The minimum X-ray flux F, in the 2-10keV range, is defined as F = 3.34*10-17*η, where η=(dP-15/dt)/(P7/2d2) and P the neutron-star rotation period.
History: From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 02-Feb-2004
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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