Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 138, Number 2, August 1999
Page(s) 253 - 266
DOI https://doi.org/10.1051/aas:1999274
Published online 15 August 1999
DOI: 10.1051/aas:1999274



Astron. Astrophys. Suppl. Ser. 138, 253-266

A search for candidate light echoes: Photometry of supernova environments[*]

F.R. Boffi - W.B. Sparks - F.D. Macchetto[*]

Send offprint request: F.R. Boffi

Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, U.S.A.
e-mail: boffi@stsci.edu, sparks@stsci.edu, macchetto@stsci.edu

Received April 19; accepted June 7, 1999

Abstract:

Supernova (SN) light echoes could be a powerful tool for determining distances to galaxies geometrically, [#!S94!#, Sparks (1994)]. In this paper we present CCD photometry of the environments of 64 historical supernovae, the first results of a program designed to search for light echoes from these SNe.

We commonly find patches of optical emission at, or close to, the sites of the supernovae. The color distribution of these patches is broad, and generally consistent with stellar population colors, possibly with some reddening. However there are in addition patches with both unusually red and unusually blue colors. We expect light echoes to be blue, and while none of the objects are quite as blue in V-R as the known light echo of SN 1991T, there are features that are unusually blue and we identify these as candidate light echoes for follow-on observations.

Key words: scattering -- supernovae: general -- distance scale

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