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Optical and ultraviolet observations of nova Vul 1987The outburst for a nova discovered in Nov. 1987 and followed since then is summarized. Although it was possible to observe it with the IUE at maximum, its ultraviolet energy faded rapidly, and after the first 2 weeks it was impossible to observe it at IUE wavelengths. It is observed to form a thick dust shell and is in the nebular stage.
Document ID
19890001340
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Starrfield, S. (Arizona State Univ. Tempe., United States)
Stryker, L. L. (Arizona State Univ. Tempe., United States)
Sonneborn, G. (IUE Observatory Lanham, MD., United States)
Sparks, Warren M. (Los Alamos National Lab. NM., United States)
Wagner, R. M. (Ohio State Univ. Columbus., United States)
Ferland, Gary (Ohio State Univ. Columbus., United States)
Gallagher, J. S. (Lowell Observatory Flagstaff, AZ., United States)
Wade, R. (Arizona State Univ. Tempe., United States)
Williams, R. E. (Cerro Tololo Inter-American Observatory La Serena (Chile)., United States)
Gehrz, Robert D. (Minnesota Univ. Minneapolis., United States)
Date Acquired
September 5, 2013
Publication Date
June 1, 1988
Publication Information
Publication: ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1
Subject Category
Astronomy
Accession Number
89N10711
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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