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The interstellar medium toward SN 1987AHigh-resolution spectra of SN 1987A obtained with the IUE satellite show absorption features from the disk and halo of the Galaxy and the LMC. A rich variety of elements and ionization states is found, including allowed resonance lines of abundant elements with ionization states ranging from C I and O I to Al III, Si IV, and C IV. The Si IV and C IV absorption at LMC velocities is unusually strong toward the supernova as compared to most other stars in the LMC and SMC. The origin of these lines is discussed.
Document ID
19880024267
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Dupree, A. K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Kirshner, R. P.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Nassiopoulos, G. E.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Raymond, J. C.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Sonneborn, G.
(NASA Goddard Space Flight Center; Computer Sciences Corp. Greenbelt, MD, United States)
Date Acquired
August 13, 2013
Publication Date
September 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 320
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
88A11494
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-16537
CONTRACT_GRANT: NAG5-841
CONTRACT_GRANT: NSG-587
Distribution Limits
Public
Copyright
Other

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