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20082020
most citedRadio-to-TeV Phase-resolved Emission from the Crab Pulsar: The Annular Gap Model

60 citations · 188 across the 10 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2013★ 41 cited

Pressure of Degenerate and Relativistic electrons in a superhigh magnetic field

Zhi Fu Gao, Wang Na, Peng Qiu He +1

Based on our previous work, we deduce a general formula for pressure of degenerate and relativistic electrons,Pe, which is suitable for superhigh magnetic fields, discuss the quant…

astro-ph.HE2012★ 19 cited

Radio and Gamma-ray Pulsed Emission from Millisecond Pulsars

YuanJie Du, GuoJun Qiao, Ding Chen

Pulsed gamma-ray emission from millisecond pulsars (MSPs) has been detected by the sensitive Fermi, which sheds light on studies of the emission region and mechanism. In particular…

astro-ph.HE2012

AXPs & SGRs: Magnetar or Quarctar?

Guojun Qiao, Xiongwei Liu, Renxin Xu +4

The concept of a "magnetar" was proposed mainly because of two factors. First, the X-ray luminosity of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) is larger…

astro-ph.HE2012

Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

YuanJie Du, GuoJun Qiao

The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish…

astro-ph.HE2012★ 60 cited

Radio-to-TeV Phase-resolved Emission from the Crab Pulsar: The Annular Gap Model

YuanJie Du, GuoJun Qiao, Wei Wang

In the framework of the three-dimensional (3D) annular gap model with reasonable parameters (the magnetic inclination angle α= 45 deg and the view angle ζ= 63 deg), we first use th…

astro-ph.HE2011★ 33 cited

Gamma-ray Emission from the Vela Pulsar Modeled with the Annular Gap and Core Gap

Y. J. Du, J. L. Han, G. J. Qiao +1

The Vela pulsar represents a distinct group of γ-ray pulsars. Fermi γ-ray observations reveal that it has two sharp peaks (P1 and P2) in the light curve with a phase separation of…