DEPENDENCE OF THE X-RAY LUMINOSITY AND PULSAR WIND NEBULA ON DIFFERENT PARAMETERS OF PULSARS AND THE EVOLUTIONARY EFFECTS-Reference-Cited by-同舟云学术

DEPENDENCE OF THE X-RAY LUMINOSITY AND PULSAR WIND NEBULA ON DIFFERENT PARAMETERS OF PULSARS AND THE EVOLUTIONARY EFFECTS

Published:2004-02 Issue:02 Volume:13 Page:197-213
ISSN:0218-2718
Container-title:International Journal of Modern Physics D
language:en
Short-container-title:Int. J. Mod. Phys. D

Author:

GUSEINOV OKTAY H.¹²,ANKAY AŞKIN¹,TAGIEVA SEVINÇ O.³,TAŞKIN M. ÖZGÜR⁴

Affiliation:

1. TÜBİTAK Feza Gürsey Institute, 81220 Çengelköy, İstanbul, Turkey

2. Akdeniz University, Physics Department, Antalya, Turkey

3. Academy of Science, Physics Institute, Baku 370143, Azerbaijan Republic

4. Middle East Technical University, Physics Department, 06531 Ankara, Turkey

Abstract

Dependences of the X-ray luminosity (Lx) of young single pulsars, due to ejection of relativistic particles, on electric field intensity, rate of rotational energy loss (Ė), magnetic field, period, and some other parameters of neutron stars are discussed. Influence of the magnetic field and effects of some other parameters of neutron stars on the Lx-Ė and the Lx-τ (characteristic time) dependences are considered. Evolutionary factors also play an important role in our considerations. Only the pulsars with L2–10 keV >1033 erg/s have pulsar wind nebula around them. The pulsars from which γ-ray radiation has been observed have low X-ray luminosity in general.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0218271804004505

Reference21 articles.

1. Re-examining the X-ray versus spin-down luminosity correlation of rotation powered pulsars

2. Astrophysics of Neutron Stars

Cited by 8 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Temporal evolution of isolated pulsars; Age-Tau problem;International Journal of Modern Physics D;2014-09

2. 1E 1207.4–5209-LIKE RADIO-QUIET NEUTRON STARS;International Journal of Modern Physics D;2009-12-15

3. How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae;Monthly Notices of the Royal Astronomical Society;2008-03

4. POSSIBLE EVOLUTION OF DIM RADIO-QUIET NEUTRON STAR 1E 1207.4-5209 BASED ON A B-DECAY MODEL;International Journal of Modern Physics D;2007-04

5. Distribution of free electrons in the galactic plane;Astrophysics;2006-04