Pulsar radio luminosity laws revisited

被引：4

作者：

Allen, MP ^{[1
]}

Horvath, JE ^{[1
]}

机构：

[1] Univ Sao Paulo, Inst Astron & Geofis, BR-04301904 Sao Paulo, Brazil

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2000年 / 317卷 / 01期

关键词：

pulsars; general;

D O I：

10.1046/j.1365-8711.2000.03481.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A luminosity law for radio pulsars was proposed by Stollman, based on features of the Ruderman-Sutherland model. We analyse that proposition in the light of the most recent data (the catalogue of Taylor, Manchester & Lyne), and perform a set of statistical tests to verify the reliability of the results. We find little evidence favouring Stollman's law, and point out a possible incompleteness of the data sets, without conclusive evidence for or against the Ruderman-Sutherland model.

引用

页码：23 / 27

页数：5

共 22 条

[1]

Bailes M., 1995, Journal of Astrophysics and Astronomy, V16, P209

[2]

Baring MG, 1997, AIP CONF PROC, P638, DOI 10.1063/1.53991

[3]

GOTTHELF EV, 1998, MEM SOC ASTRON ITAL, V69, P831

[4] ON NATURE OF PULSARS .3. ANALYSIS OF OBSERVATIONS [J].

GUNN, JE ;

OSTRIKER, JP .

ASTROPHYSICAL JOURNAL, 1970, 160 (03) :979-&

[5] An x-ray pulsar with a superstrong magnetic field in the soft γ-ray repeater SGR1806-20 [J].

Kouveliotou, C ;

Dieters, S ;

Strohmayer, T ;

van Paradijs, J ;

Fishman, GJ ;

Meegan, CA ;

Hurley, K ;

Kommers, J ;

Smith, I ;

Frail, D ;

Murakami, T .

NATURE, 1998, 393 (6682) :235-237

[6] THE GALACTIC POPULATION OF PULSARS [J].

LYNE, AG ;

MANCHESTER, RN ;

TAYLOR, JH .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1985, 213 (03) :613-639

[7]

Malov I. F., 1995, Astronomy Reports, V39, P503

[8]

Malov I. F., 1995, Astronomy Reports, V39, P510

[9]

MALOV IF, 1985, SVA, V29, P335

[10]

Manchester R.N., 1977, PULSARS

← 1 2 3 →