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Kinematics of Oxygen-Rich Filaments in Puppis A

Published online by Cambridge University Press:  12 April 2016

P. Frank Winkler
Affiliation:
Middlebury College, Middlebury, VT, U.S.A.
John H. Tuttle
Affiliation:
Middlebury College, Middlebury, VT, U.S.A.
Robert P. Kirshner
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, U.S.A.
Michael J. Irwin
Affiliation:
Institute of Astronomy, Cambridge University, Cambridge, U.K.

Abstract

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We have measured proper motions for fast, oxygen-rich knots in Puppis A, which we demonstrate are probably uncontaminated ejecta from the progenitor star’s core. Typical fast knots show motions of 0.1-0.2 arcsec yr-1 diverging from a point 4’ northeast of the center of the radio shell. A model assuming constant expansion fits the data well and gives an age of 3700 ± 300 yr for Puppis A. We also present new spectra which indicate the presence of neon along with oxygen in the fast knots.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1988

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