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Late-time spectra and type Ia supernova models: New clues from the Hubble Space TelescopeCalculated late-time spectra of two classical hydrodynamical models for Type Ia supernovae (deflagration model W7 of Nomoto, Thielemann, & Yokoi, and delayed detonation model DD4 of Woosley & Weaver) are compared with observations of SN 1992A and other spectroscopically normal SNe Ia. An important new piece of information is provided by observations done with the Hubble Space Telescope (HST) which cover the ultraviolet range at the nebular phase of a SN Ia: SN 1992A in NGC 1380. For the first time a picture of SN Ia emission from the ultraviolet through the optical is obtained at these phases. Predictions of the classical model (W7 and DD4) are compared with the observed spectrum of SN 1992A and with the optical spectra of SN 1989M in NGC 4579 and SN 1990N in NGC 4639 at similar epochs. The absolute B and V magnitudes of the models are also estimated at these late phases. Taken at face value the nebular spectra of these 'classical' models are more consistent with the long extragalactic distance scale, pointing to distances to NGC 4579 around 21 +/- 3 Mpc and a slightly larger distance, 22 +/- 3 Mpc, to NGC 4639, on the back side of the Virgo Cluster. However, the calculated Fe(+3) luminosity as predicted from the models exceeds the observed limit from the HST data of SN 1992A. Other differences in the ratios of the line intensities between calculated and observed spectra, show some disagreement with the observed spectra at the nebular phases. They may not be the best choice for spectroscopically normal SNe Ia, and their use as an independent calibration of the extragalactic distance scale should be viewed with caution.
Document ID
19950051847
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ruiz-Lapuente, P.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Kirshner, R. P.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Phillips, M. M.
(Cerro Tololo Inter-American Observatory La Serena, Chile)
Challis, P. M.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Schmidt, B. P.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA United States)
Filippenko, A. V.
(University of California, Berkeley, CA United States)
Wheeler, J. C.
(University of Texas, Austin, TX United States)
Date Acquired
August 16, 2013
Publication Date
January 20, 1995
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 439
Issue: 1
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
95A83446
Funding Number(s)
CONTRACT_GRANT: NAS5-26555
CONTRACT_GRANT: NSF AST-92-18475
Distribution Limits
Public
Copyright
Other

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