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Title:
Highest velocity ejecta of Cassiopeia A
Authors:
Fesen, Robert A.; Becker, Robert H.; Goodrich, Robert W.
Affiliation:
AA(Colorado, University, Boulder), AB(California, University, Davis; Lawrence Livermore National Laboratory, Livermore), AC(Lick Observatory, Santa Cruz, CA)
Publication:
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 329, June 15, 1988, p. L89-L92. (ApJL Homepage)
Publication Date:
06/1988
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Cassiopeia A, Nitrogen, Optical Emission Spectroscopy, Stellar Envelopes, Stellar Mass Ejection, Supernova Remnants, Abundance, Charge Coupled Devices, Forbidden Transitions, Radial Velocity, Radio Sources (Astronomy), Stellar Mass
DOI:
10.1086/185183
Bibliographic Code:
1988ApJ...329L..89F

Abstract

CCD interference-filter images and spectroscopy of Cassiopeia A's outlying optical emission knots are presented. Six new high-velocity forbidden N II-emitting knots are identified, which increases the total now known to 15. New spectra of seven of these knots suggest high N abundances. Spectra, radial velocity, and proper motion data indicate that these outlying knots possess ejection velocities between 7000 and 8600 km/s and are probably material from the progenitor's outer layers. These observations suggest that the Cas A supernova had a maximum expansion velocity of at least 8500 km/s, a substantial nitrogen-rich but hydrogen-deficient envelope, an explosion date around A.D. 1680, and a W progenitor. Cas A's northeastern emission jet, which consists of sulfur-rich ejecta, appears to be an isolated, well-collimated structure extending at least 265 arcsec from the remnant center. Such radial distances imply ejection velocities of up to 11,000 km/s and at least a partially asymmetric stellar disruption.

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