X-ray Observations of the Tycho Supernova Remnant

Details X-ray Observations of the Tycho Supernova Remnant X-ray Observations of the Tycho Supernova Remnant

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...208.5906h&link_type=abstract

American Astronomical Society Meeting 208, #59.06; Bulletin of the American Astronomical Society, Vol. 38, p.139

Physics

Scientific paper

In this presentation I summarize some key new findings from recent Chandra and XMM-Newton data on the remnant of the supernova (SN) observed by Tycho Brahe in 1572, which is widely believed to have been of Type Ia origin. Studies of the Tycho supernova remnant (SNR) at the current epoch address aspects of SN Ia physics, the evolution of young SNRs, and cosmic ray acceleration at high Mach-number shocks.Research on the Tycho SNR at Rutgers has been supported by Chandra grants GO3-4066X and AR5-6010X.

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