Abstract
The discovery of the γ-ray pulsar PSR J1836+5925, powering the formerly unidentified EGRET source 3EG J1835+5918, was one of the early accomplishments of the Fermi Large Area Telescope (LAT). Sitting 25° off the Galactic plane, PSR J1836+5925 is a 173ms pulsar with a characteristic age of 1.8 million years, a spindown luminosity of 1.1 × 1034erg s-1, and a large off-peak (OP) emission component, making it quite unusual among the known γ-ray pulsar population. We present an analysis of one year of LAT data, including an updated timing solution, detailed spectral results, and a long-term light curve showing no indication of variability. No evidence for a surrounding pulsar wind nebula is seen and the spectral characteristics of the OP emission indicate it is likely magnetospheric. Analysis of recent XMM-Newton observations of the X-ray counterpart yields a detailed characterization of its spectrum, which, like Geminga, is consistent with that of a neutron star showing evidence for both magnetospheric and thermal emission.
Original language | English |
---|---|
Pages (from-to) | 1209-1218 |
Number of pages | 10 |
Journal | Astrophysical Journal |
Volume | 712 |
Issue number | 2 |
DOIs | |
Publication status | Published - 2010 |
Keywords
- Gamma rays: general
- Pulsars: general
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science