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Cited article:

On the age of PSR B 1509-58

V. V. Gvaramadze

A&A, 374 1 (2001) 259-263

Published online: 2001-07-15

DOI: https://doi.org/10.1051/0004-6361:20010720

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Neutron Stars in Supernova Remnants and Beyond

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On the origin of the system PSR B 1757$\mathsf{-}$24/SNR G 5.4$\mathsf{-}$1.2

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Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS

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PSR B 1706-44 and the SNR G 343.1-2.3 as the remnants of a cavity supernova explosion

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WR 120bb and WR 120bc: a pair of WN9h stars with possibly interacting circumstellar shells

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Point X-ray sources in the SNR G 315.4-2.30 (MSH 14-63, RCW 86)

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Observation of an Extended Very High Energy Gamma‐Ray Emission from MSH 15‐52 with CANGAROO‐III

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ChandraImaging of the X‐Ray Nebula Powered by Pulsar B1509−58

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Pulsar Spin-down by a Fallback Disk and the [ITAL]P[/ITAL]-[FORMULA][F][A][AC]P[/AC][AC][d2][/AC][/A][/F][/FORMULA] Diagram

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Disk-assisted Spin-down of Young Radio Pulsars

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