Center-filled Supernova Remnant G16.85-1.05 and its surroundings

Physics

Scientific paper

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Chandra Proposal Id #05500054

Scientific paper

In one pointing we will image 5 sources: an SNR, a microquasar, a
pulsar, an unidentified ASCA source and a Wolf-Rayet star. Our primary
goal is to resolve a pulsar-wind nebula in the SNR G16.85-1.05. As a
by-product, we will obtain a high quality spectrum of the microquasar LS
5039 and possibly detect X-ray emission from the PSR J1825-1446.

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