Journal
ASTROPHYSICAL JOURNAL
Volume 631, Issue 1, Pages 480-487Publisher
IOP PUBLISHING LTD
DOI: 10.1086/432527
Keywords
gamma rays : observations; pulsars : individual (PSR B1706-44)
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We report on Chandra ACIS imaging of the pulsar wind nebula (PWN) of the young Vela-like PSR B1706-44, which shows the now common pattern of an equatorial wind and polar jets. The structure is particularly rich, showing a relativistically boosted termination shock, jets with strong confinement, a surrounding radio/X-ray PWN, and evidence for a quasistatic bubble nebula.'' The structures trace the pulsar spin geometry and illuminate its possible relation to SNR G343.1-2.3. We also obtain improved estimates of the pulsar flux and nebular spectrum, constraining the system age and energetics.
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