A pulsar wind nebula in G18.95-1.1?

Details A pulsar wind nebula in G18.95-1.1? A pulsar wind nebula in G18.95-1.1?

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2590t&link_type=abstract

Chandra proposal ID #10500739

Computer Science

Scientific paper

We propose to observe the central region of the composite SNR G18.95-1.1. Although this object has been extensively observed in the radio regime and to a minor extent in X-rays with ASCA and ROSAT, all searches for a point source have been unsuccessful. Our motivation to observe the G18.95-1.1 with Chandra is to detect an X-ray point source and perhaps non-thermal diffuse emission which could be the putative pulsar and its wind nebula. For this objective, high resolution observations are necessary to pinpoint the location of the source, making Chandra the only X-ray mission which with this study can be carried out.

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