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Early observations of the nearby Type Ia supernova SN 2015F

Cartier, R., Sullivan, M., Firth, R. E., Pignata, G., Mazzali, P., Maguire, K., Childress, M. J., Arcavi, I., Ashall, C., Bassett, B., Crawford, S. M., Frohmaier, C., Galbany, L., Gal-Yam, A., Hosseinzadeh, G., Howell, D. A., Inserra, C., Johansson, J., Kasai, E. K., McCully, C., Prajs, S., Prentice, S., Schulze, S., Smartt, S. J., Smith, K. W., Smith, M., Valenti, S. and Young, D. R. 2017. Early observations of the nearby Type Ia supernova SN 2015F. Monthly Notices of the Royal Astronomical Society 464 (4) , pp. 4476-4494. 10.1093/mnras/stw2678

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Abstract

We present photometry and time series spectroscopy of the nearby Type Ia supernova (SN Ia) SN 2015F over −16 d to +80 d relative to maximum light, obtained as part of the Public ESO Spectroscopic Survey of Transient Objects. SN 2015F is a slightly sub-luminous SN Ia with a decline rate of Δm15(B) = 1.35 ± 0.03 mag, placing it in the region between normal and SN 1991bg-like events. Our densely sampled photometric data place tight constraints on the epoch of first light and form of the early-time light curve. The spectra exhibit photospheric C ii λ6580 absorption until −4 days, and high-velocity Ca ii is particularly strong at <−10 d at expansion velocities of ≃23 000 km s−1. At early times, our spectral modelling with syn++ shows strong evidence for iron-peak elements (Fe ii, Cr ii, Ti ii, and V ii) expanding at velocities >14 000 km s−1, suggesting mixing in the outermost layers of the SN ejecta. Although unusual in SN Ia spectra, including V ii in the modelling significantly improves the spectral fits. Intriguingly, we detect an absorption feature at ∼6800 Å that persists until maximum light. Our favoured explanation for this line is photospheric Al ii, which has never been claimed before in SNe Ia, although detached high-velocity C ii material could also be responsible. In both cases, the absorbing material seems to be confined to a relatively narrow region in velocity space. The nucleosynthesis of detectable amounts of Al ii would argue against a low-metallicity white dwarf progenitor. We also show that this 6800 Å feature is weakly present in other normal SN Ia events and common in the SN 1991bg-like sub-class.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Publisher: Oxford University Press
ISSN: 0035-8711
Date of First Compliant Deposit: 23 January 2019
Date of Acceptance: 19 October 2016
Last Modified: 30 Jan 2019 12:00
URI: http://orca.cf.ac.uk/id/eprint/118667

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