Add to ORKGWe present a statistical analysis of the X-ray luminosity of rotation-powered pulsars and their surrounding nebulae using the sample of Kargaltsev & Pavlov, and we complement this with an analysis of the γ -ray emission of Fermi-detected pulsars. We report a strong trend in the efficiency with which spin-down power is converted to X-ray and γ -ray emission with characteristic age: young pulsars and their surrounding nebulae are efficient X-ray emitters, whereas in contrast old pulsars are efficient γ -ray emitters. We divided the X-ray sample in a young (τc <1.7 × 104 yr) and old sample and used linear regression to search for correlations between the logarithm of the X-ray and γ -ray luminosities and the logarithms of the periods and perio...
The population of young, non-recycled pulsars with spin-down energies |$\dot{E} \gt 10^{35}$| erg s^...
The general properties of the nonthermal nonpulsed X-ray emission of rotation-powered pulsars are in...
We study the properties of the pulsed component of hard (>2 keV) X-ray emission from pulsars based o...
(6 pages, 2 figures)Pulsar wind nebulae are a prominent class of very high energy (E > 0.1 TeV) Gala...
We investigate radio emission efficiency, xi, of pulsars and report a near-linear inverse correlatio...
We use a new self-consistent model to derive the conversion efficiency from rotation power to γ-ray ...
We present a statistical study of the nonthermal X-ray emission of 27 young rotation-powered pulsars...
International audienceThe very high energy γ-ray spectra of Pulsar Wind Nebulae are interpreted as d...
Due to recent observations with ROSAT and ASCA the number of rotation-powered pulsars seen at X-ray ...
We study statistical properties of the Galactic population of X-ray pulsars with ages of less than 1...
Based on our self-consistent outer gap model for high energy emission from the rotationpowered pulsa...
The Fermi Large Area Telescope has revealed that rotation powered millisecond pulsars (MSPs) are a m...
Using available multiwavelength data for the pulsars of different ages detected in the optical range...
This thesis focuses on the radiation mechanisms of non-thermal X-rays and soft gamma-rays of two typ...
The population of young, non-recycled pulsars with spin-down energies |$\dot{E} \gt 10^{35}$| erg s^...
The general properties of the nonthermal nonpulsed X-ray emission of rotation-powered pulsars are in...
We study the properties of the pulsed component of hard (>2 keV) X-ray emission from pulsars based o...
(6 pages, 2 figures)Pulsar wind nebulae are a prominent class of very high energy (E > 0.1 TeV) Gala...
We investigate radio emission efficiency, xi, of pulsars and report a near-linear inverse correlatio...
We use a new self-consistent model to derive the conversion efficiency from rotation power to γ-ray ...
We present a statistical study of the nonthermal X-ray emission of 27 young rotation-powered pulsars...
International audienceThe very high energy γ-ray spectra of Pulsar Wind Nebulae are interpreted as d...
Due to recent observations with ROSAT and ASCA the number of rotation-powered pulsars seen at X-ray ...
We study statistical properties of the Galactic population of X-ray pulsars with ages of less than 1...
Based on our self-consistent outer gap model for high energy emission from the rotationpowered pulsa...
The Fermi Large Area Telescope has revealed that rotation powered millisecond pulsars (MSPs) are a m...
Using available multiwavelength data for the pulsars of different ages detected in the optical range...
This thesis focuses on the radiation mechanisms of non-thermal X-rays and soft gamma-rays of two typ...
The population of young, non-recycled pulsars with spin-down energies |$\dot{E} \gt 10^{35}$| erg s^...
The general properties of the nonthermal nonpulsed X-ray emission of rotation-powered pulsars are in...
We study the properties of the pulsed component of hard (>2 keV) X-ray emission from pulsars based o...