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Observations and simulations of nova Vul 1984 no. 2: A nova with ejecta rich in oxygen, neon, and magnesiumNova Vul 1984 no. 2 was observed with IUE from Dec. 1984 through Nov. 1987. The spectra are characterized by strong lines from Mg, Ne, C, Si, O, N, and other elements. Data obtained in the ultraviolet, infrared, and optical show that this nova is ejecting material rich in oxygen, neon, and magnesium.
Document ID
19890001338
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Starrfield, S. (Arizona State Univ. Tempe., United States)
Sonneborn, G. (IUE Observatory Lanham, MD., United States)
Stryker, L. L. (Arizona State Univ. Tempe., United States)
Sparks, Warren M. (Los Alamos National Lab. NM., United States)
Truran, James W. (Illinois Univ. Urbana., United States)
Ferland, Gary (Ohio State Univ. Columbus., United States)
Wagner, R. M. (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)
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
89N10709
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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