Evidence for a High-Velocity Carbon-rich Layer in the Type Ia SN 1990N

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©1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Adam Fisher et al 1997 ApJ 481 L89 DOI 10.1086/310660

1538-4357/481/2/L89

Abstract

We use a parameterized spectrum-synthesis code to make a direct analysis of a high quality spectrum of the Type Ia SN 1990N that was obtained by Leibundgut et al. 14 days before the time of optical maximum. We suggest that the absorption feature observed near 6040 Å, which has been attributed to blueshifted λ6355 of Si II, actually was produced by blueshifted λ6580 of C II, in a high-velocity (v > 26, 000 km s-1) carbon-rich region. Implications for SN Ia explosion models are briefly discussed.

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10.1086/310660