Multiwavelength Monitoring Of The Luminous Accreting X-ray Sources And SN 1978K In NGC 1313

Details Multiwavelength Monitoring Of The Luminous Accreting X-ray Sources And SN 1978K In NGC 1313 Multiwavelength Monitoring Of The Luminous Accreting X-ray Sources And SN 1978K In NGC 1313

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.4803s&link_type=abstract

American Astronomical Society, AAS Meeting #211, #48.03; Bulletin of the American Astronomical Society, Vol. 39, p.809

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The nearby barred spiral galaxy NGC 1313 contains three ultraluminous X-ray sources (two accreting binaries and the unusual ultraluminous Type IIn supernova SN 1978K) as well as other bright persistent and transient X-ray sources. Here we will discuss our radio (Australia Telescope Compact Array and Australian Long Baseline Array) and X-ray (XMM-Newton) monitoring observations of NGC 1313.

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