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 2003PAZh...29..571M
=2003AstL...29..502M 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:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table.dat 30 155 Pulsars with η≥24
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See also:
J/AZh/71/762 : Radio luminosities of 232 pulsars (Malov+, 1994)
Byte-by-byte Description of file: table.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Seq Sequential number
4 A1 --- n_Seq [*] *: pulsar with measured X-ray fluxes
(Possenti et al., 2002A&A...387..993P 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)
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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.
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History:
From electronic version of the journal
(End) James Marcout, Patricia Bauer [CDS] 02-Feb-2004