Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

RADIO AND GAMMA-RAY PULSED EMISSION FROM MILLISECOND PULSARS

Journal Article · · Astrophysical Journal
;  [1]
  1. National Space Science Center, Chinese Academy of Sciences, No.1 Nanertiao, Zhongguancun, Haidian District, Beijing 100190 (China)
Pulsed {gamma}-ray emission from millisecond pulsars (MSPs) has been detected by the sensitive Fermi space telescope, which sheds light on studies of the emission region and its mechanism. In particular, the specific patterns of radio and {gamma}-ray emission from PSR J0101-6422 challenge the popular pulsar models, e.g., outer gap and two-pole caustic models. Using the three-dimensional annular gap model, we have jointly simulated radio and {gamma}-ray light curves for three representative MSPs (PSR J0034-0534, PSR J0101-6422, and PSR J0437-4715) with distinct radio phase lags, and present the best simulated results for these MSPs, particularly for PSR J0101-6422 with complex radio and {gamma}-ray pulse profiles, and for PSR J0437-4715 with a radio interpulse. We have found that both the {gamma}-ray and radio emission originate from the annular gap region located in only one magnetic pole, and the radio emission region is not primarily lower than the {gamma}-ray region in most cases. In addition, the annular gap model with a small magnetic inclination angle instead of an 'orthogonal rotator' can account for the MSPs' radio interpulse with a large phase separation from the main pulse. The annular gap model is a self-consistent model not only for young pulsars but also MSPs, and multi-wavelength light curves can be fundamentally explained using this model.
OSTI ID:
22167222
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 763; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

Modeling Phase-Aligned Gamma-Ray And Radio Millisecond Pulsar Light Curves
Journal Article · Sun Dec 11 19:00:00 EST 2011 · The Astrophysical Journal · OSTI ID:1356768

MODELING PHASE-ALIGNED GAMMA-RAY AND RADIO MILLISECOND PULSAR LIGHT CURVES
Journal Article · Sat Dec 31 23:00:00 EST 2011 · Astrophysical Journal · OSTI ID:22004349

FIVE NEW MILLISECOND PULSARS FROM A RADIO SURVEY OF 14 UNIDENTIFIED FERMI-LAT GAMMA-RAY SOURCES
Journal Article · Tue Mar 20 00:00:00 EDT 2012 · Astrophysical Journal Letters · OSTI ID:22047975