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The Copernicus ultraviolet spectral atlas of Gamma PegasiAn ultraviolet spectral atlas is presented for the B2 IV star Gamma Pegasi, which has been scanned from 970 to 1501 A by the Princeton spectrometer aboard the Copernicus satellite. From 970 to 1430 A the observations have a nominal resolution of 0.05 A. At the longer wavelengths the resolution is 0.1 A. The atlas is presented in graphs. Line identifications are also listed.
Document ID
19850049271
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/191026
Authors
Rogerson, J. B., Jr. (Princeton University New Observatory, Princeton, NJ, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1985
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 57
ISSN: 0067-0049
Subject Category
Astronomy
Accession Number
85A31422
Funding Number(s)
CONTRACT_GRANT: NAS5-23576
CONTRACT_GRANT: NAGW-477
Distribution Limits
Public
Copyright
Other

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