Historical Supernovae and Their Remnants

By F. Stephenson, Douglas R. Green. 2002

244 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/828ad8061505f727e7fc8543f83ddc535bf0f3e2

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Citations in the corpus

The evolution and structure of pulsar wind nebulae (2006, background): “4The association of 3C 58 with 1181 CE is not completely secure; see Stephenson & Green (2002) and Chevalier (2005), and references therein.”
OBSERVING THE NEXT GALACTIC SUPERNOVA (2013, background): “Stephenson & Green (2002) conclude that 5 Galactic SNe have been observed since 1000 AD, when the historical records become relatively complete.”
Observational Clues to the Progenitors of Type Ia Supernovae (2013, background): “SN 1006 is widely considered a likely SN Ia, based on its 500 pc height above the Galactic plane, its symmetry, and the absence of a neutron star (Stephenson & Green 2002).”
A revised catalogue of 294 Galactic supernova remnants (2019, background): “Previous versions have been published in (Green 1984, 1988, 1991; Stephenson & Green 2002; Green 2004, 2009, 2014).”
A revised Galactic supernova remnant catalogue (2009, background): “Introduction Over the last twenty five years I have produced several published versions of a catalogue of Galactic SNRs (Green 1984, 1988, 1991; Stephenson & Green 2002; Green 2004), along with more detailed web-based versions (most recently in 2006).”
A catalogue of 294 Galactic supernova remnants (2014, methodology): “An alternative term used toescribe such remnants is ‘mixed morphology’, see Rho & Petre 1998.)”
Young Core-Collapse Supernova Remnants and Their Supernovae (2004, background): “Of the historical supernovae prior to 1500A.D., SN 1054 and SN 1006 have the most secure identifications with SNRs; in addition to positional agreement, the expansion of the remnants is consistent with the implied ages (Stephenson & Green 2002).”
A census of high-energy observations of Galactic supernova remnants (2012, background): “6%) – 10 other cases are kept in the database for the record but are considered unlikely. 3.1.2. Historicalevents The database also contains a table of 14 records of the sighting of a supernova (SN) (Green, 2002; Green and Stephenson, 2003): • 5 certain events (in 1604, 1572, 1181, 1054, 1006); • 4 ”