Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20915616t&link_type=abstract
2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #156.16; Bulletin of the American Astronomical Society,
Astronomy and Astrophysics
Astronomy
Scientific paper
G292.0+1.8 is an oxygen-rich supernova remnant (SNR)--a member of the same exclusive family as Cas A. It is the only Galactic SNR which displays all the features expected in the young remnant of a core-collapse supernova: optical (and X-ray) emission from fragments of metal-rich ejecta, an active pulsar and associated pulsar-wind nebula, and evidence for interaction of a blast wave with circumstellar wind material. We report here measurements of proper motions of the ejecta-dominated filaments, based on CCD images in the [O III] 5007 Å line taken from the CTIO 0.9m telescope at epochs from 1999 through 2006. We also use additional images from as early as 1986 for the central region of this 8-arcmin-diameter remnant. Matched narrow-band continuum images at most epochs aid in removing the myriad stars that litter the crowded field, making small, faint filaments of ejecta more apparent. We use a two-dimensional cross-correlation technique to measure the shifts for dozens of individual filaments between multiple epoch pairs. The fastest, most outlying filaments display proper motions as large as 0.15 arcsec/yr. Preliminary results appear consistent with undecelerated expansion from a common center, and suggest a kinematic age slightly younger than the 3000-3400 yr inferred by Ghavamian et al. (2005, ApJ, 635, 365) from Fabry-Perot measurements of the radial velocities for many of the ejecta filaments in G292.
This work is partially supported by the National Science Foundation through grant AST-0307613.
Long Knox S.
Reith Claudine N.
Twelker Karl
Winkler Frank P.
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