Radio and X-ray nebulae associated with PSR J1509-5850

Details Radio and X-ray nebulae associated with PSR J1509-5850 Radio and X-ray nebulae associated with PSR J1509-5850

2007-04-10

arxiv.org/abs/0704.1265v2

Astronomy and Astrophysics

Astrophysics

Accepted by A&A, 5 pages, 4 figures, 1 table

Scientific paper

10.1051/0004-6361:20077628

We have discovered a long radio trail at 843 MHz which is apparently associated with middle age pulsar PSR J1509-5850. The radio trail has a length of ~7 arcmin. In X-rays, Chandra observations of PSR J1509-5850 reveal an associated X-ray trail which extends in the same orientation as the radio trail. Moreover, two clumpy structures are observed along the radio trail. The larger one is proposed to be the supernova remnant (SNR) candidate MSC 319.9-0.7. Faint X-ray enhancement at the position of the SNR candidate is found in the Chandra data.

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