Confirming and exploring the supernova remnant candidate G308.3-1.4

Details Confirming and exploring the supernova remnant candidate G308.3-1.4 Confirming and exploring the supernova remnant candidate G308.3-1.4

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cxo..prop.2843h&link_type=abstract

Chandra proposal ID #11500804

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Scientific paper

ROSAT all-sky survey (RASS) data have provided another window to search for supernova remnants (SNRs). Utilizing this database, the first catalogue of extended X-ray sources as promising SNR candidates was published ten years ago. However, these targets have not yet been fully explored by the state-of-art X-ray observatories. We have reexamined this catalogue and chosen the brightest SNR candidate, G308.3-1.4, for a detailed spectro-imaging X-ray study with Chandra. We propose a short ACIS-I imaging observation to have a full coverage of G308.3-1.4 in order to investigate its spectrum and morphology in details as well as to search for the associated compact stellar remnants produced in the supernova explosion.

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