Fesen, R. A., Hammell, M. C., Morse, J., Chevalier, R. A., Borkowski, K. J., Dopita, M. A., Gerardy, C. L., Lawrence, S. S., Raymond, J. C., van den Bergh, S. (July 2006) The expansion asymmetry and age of the Cassiopeia A supernova remnant. Astrophysical Journal, 645 (1). pp. 283-292. ISSN 0004-637X
Preview |
PDF (Paper)
Hammell Astrophysical J 2006b.pdf - Published Version Download (1MB) | Preview |
Abstract
HST images of the young supernova remnant Cas A are used to explore the expansion and spatial distribution of its highest velocity debris. ACS WFC images taken in 2004 March and December with Sloan F625W, F775W, and F850LP filters were used to identify 1825 high-velocity, outlying ejecta knots through measured proper motions of 0."35 - 0."90 yr(-1), corresponding to V-trans = 5500-14,500 km s(-1) assuming d = 3.4 kpc. The distribution of derived transverse expansion velocities for these ejecta knots shows a striking bipolar asymmetry with the highest velocity knots (V-trans >= 10,500 km s(-1)) confined to nearly opposing northeast and southwest "jets'' at P.A. = 45 degrees-70 degrees and 230 degrees-270 degrees, respectively. The jets have about the same maximum expansion velocity of similar or equal to 14,000 km s(-1) and appear kinematically and chemically distinct in that they are the remnant's only S-rich ejecta with expansion velocities above the 10,000-11,000 km s(-1) exhibited by outer nitrogen-rich ejecta, which otherwise represent the remnant's highest velocity debris. In addition, we find significant gaps in the spatial distribution of outlying ejecta in directions that are approximately perpendicular to the jets (P.A. = 145 degrees-200 degrees and 335 degrees-350 degrees). The remnant's central X-ray point source lies some 700 to the southeast of the estimated expansion center ( P.A. = 169 degrees +/- 8.degrees 4) indicating a projected motion toward the middle of the broad southern ejecta knot gap. Extrapolations of measured 9 month proper motions for all 1825 outer ejecta knots and a selected subsample of 72 bright and compact knots suggest explosion dates (assuming no knot deceleration) of 1662 +/- 27 and 1672 +/- 18, respectively. We find some evidence for nonuniform deceleration in different directions around the remnant and find 126 knots located along the northwestern limb among the least decelerated ejecta, suggesting a convergence date of 1681 +/- 19. A remnant age of around 325 yr would imply a +/- 350 km s(-1) transverse velocity for the central X-ray point source.
| Item Type: | Paper |
|---|---|
| Uncontrolled Keywords: | ISM : individual (Cassiopeia A) ISM : kinematics and dynamics supernova remnants CORE-COLLAPSE SUPERNOVAE GAMMA-RAY BURSTS X-RAY NEUTRON-STAR PULSAR KICKS PROPER MOTIONS POINT-SOURCE SHOCK-WAVES RICH EJECTA EXPLOSIONS Astronomy & Astrophysics |
| Subjects: | physics |
| CSHL Authors: | |
| Communities: | CSHL labs > Hammell M. lab |
| Depositing User: | Matt Covey |
| Date: | July 2006 |
| Date Deposited: | 06 Nov 2014 19:44 |
| Last Modified: | 06 Nov 2014 19:44 |
| URI: | https://repository.cshl.edu/id/eprint/30888 |
Actions (login required)
 |
Administrator's edit/view item |
