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Astrophysical Journal, ISSN 0004-637X, 12/2018, Volume 868, Issue 2, p. 119
PSR J1809-1917 is a young (tau = 51 kyr) energetic (<(E)over dot> = 1.8 x 10(36) erg s(-1)) radio pulsar powering a pulsar wind nebula (PWN). We report on the... 
pulsars: individual (PSR J1809-1917) | X-rays: general | ISM: individual objects (HESS J1809193) | stars: neutron | VARIABILITY | HUBBLE-SPACE-TELESCOPE | ASTRONOMY & ASTROPHYSICS | ISM: individual objects (HESS J1809-193) | RADIO | X-RAY NEBULA | EMISSION | MOVING WISPS | DISCOVERY | Physics - High Energy Astrophysical Phenomena
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