Published April 20, 1990
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Journal Article
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A nova-like red variable in M31
Chicago
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Abstract
A late-type supergiant which appeared in the bulge of M31 in the last observing season faded 3 bolometric magnitudes in 100 days and is now no longer detectable. It is suggested that the object was a nova of an unusual type.
Additional Information
© American Astronomical Society • Provided by the NASA Astrophysics Data System. Received 1989 November 14; accepted 1990 February 7. We are grateful to Don Schneider for reducing the spectrum shown in Figure 4 and to Jay Gallagher for reviewing the manuscript. Partial support for this work was provided by NSF grants AST 86-13059 and 87-21705 to Caltech.Attached Files
Published - 1990ApJ___353L__35M.pdf
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1990ApJ___353L__35M.pdf
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Additional details
- Eprint ID
- 96076
- Resolver ID
- CaltechAUTHORS:20190603-153224067
- NSF
- AST 86-13059
- NSF
- AST 87-21705
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2019-06-04Created from EPrint's datestamp field
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2021-11-16Created from EPrint's last_modified field