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A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf

By Andrea Pastorello and others
We present the results of the monitoring campaign of the Type IIn supernova (SN) 2018cnf (aka ASASSN-18mr). It was discovered about 10 days before the maximum light (on MJD = 58293.4+-5.7 in the V band, with MV = -18.13+-0.15 mag). The multiband light curves show an immediate post-peak decline with... Show more
September 3, 2019
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A luminous stellar outburst during a long-lasting eruptive phase first, and then SN IIn 2018cnf
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