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Searching for swept-up hydrogen and helium in the late-time spectra of 11 nearby Type Ia supernovae

Maguire, K, Taubenberger, S, Sullivan, M and Mazzali, PA (2016) Searching for swept-up hydrogen and helium in the late-time spectra of 11 nearby Type Ia supernovae. Monthly Notices of the Royal Astronomical Society, 457 (3). pp. 3254-3265. ISSN 0035-8711

Searching_for_swept-up_hydrogen_and_helium_in_the_late-time_spectra_of_11_nearby_Type_Ia_supernovae.pdf - Published Version

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The direct detection of a stellar system that explodes as a Type Ia supernova (SN Ia) has not yet been successful. Various indirect methods have been used to investigate SN Ia progenitor systems but none have produced conclusive results. A prediction of single-degenerate models is that H- (or He-) rich material from the envelope of the companion star should be swept up by the SN ejecta in the explosion. Seven SNe Ia have been analysed to date looking for signs of H-rich material in their late-time spectra and none were detected. We present results from new late-time spectra of 11 SNe Ia obtained at the Very Large Telescope using XShooter and FORS2. We present the tentative detection of Hα emission for SN 2013ct, corresponding to ∼0.007 M⊙ of stripped/ablated companion star material (under the assumptions of the spectral modelling). This mass is significantly lower than expected for single-degenerate scenarios, suggesting that >0.1 M⊙ of H-rich is present but not observed. We do not detect Hα emission in the other 10 SNe Ia. This brings the total sample of normal SNe Ia with non-detections (<0.001–0.058 M⊙) of H-rich material to 17 events. The simplest explanation for these non-detections is that these objects did not result from the explosion of a CO white dwarf accreting matter from a H-rich companion star via Roche lobe overflow or symbiotic channels. However, further spectral modelling is needed to confirm this. We also find no evidence of He-emission features, but models with He-rich companion stars are not available to place mass limits.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: 0201 Astronomical And Space Sciences
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press
Related URLs:
Date Deposited: 18 Oct 2017 10:51
Last Modified: 04 Sep 2021 11:05
DOI or ID number: 10.1093/mnras/stv2991
URI: https://researchonline.ljmu.ac.uk/id/eprint/7375
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