Abstract
We report on Chandra imaging observations of the Galactic unidentified γ-ray source GeV J1809-2327, comparing the X-ray images with new VLA 1.46 and 4.86 GHz maps. The X-ray images reveal a point source connected to a nonthermal X-ray/radio nebula, supporting a pulsar/wind model for the γ-ray emitter. We also detect numerous X-ray sources from the young stellar association in the adjacent H II region S32.
Original language | English (US) |
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Pages (from-to) | L91-L95 |
Journal | Astrophysical Journal |
Volume | 565 |
Issue number | 2 II |
DOIs | |
State | Published - Feb 1 2002 |
Keywords
- Gamma rays: observations
- Pulsars: general
- Supernova remnants
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science