G29.7-0.3: a Supernova Remnant like it Otta BE

Details G29.7-0.3: a Supernova Remnant like it Otta BE G29.7-0.3: a Supernova Remnant like it Otta BE

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..126h&link_type=abstract

Chandra Proposal ID #01500674

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Chandra Proposal Id #01500674

Scientific paper

In our quest for an understanding of neutron star birth properties, we have but two examples of young neutron stars: the Crab and 0540-69 in the LMC. We seek to find a third in 3C58 (SN1181) in a companion proposal, and may hope to see a fourth emerge in SN1987A during AXAF's lifetime. Here, we propose to search for another in G29.7-0.3, a remnant on the other side of the Galaxy which exhibits an intense central synchrotron nebula surrounded by a bright, 2' shell of thermal emission. ASCA observations clearly establish the two emission components, but are completely incapable of spatially resolving them or allowing the search for a central point source. This object is an AXAF "poster remnant", an SNR like it otta be.

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