http://arxiv.org/abs/1605.07382
We propose that two recent intermediate luminosity optical transients (ILOTs), M31LRN 2015 and SNHunt 275 (PTF 13efv) can be accounted for with a stellar binary model involving mass transfer that leads to the launching of jets. We inspect observations of the ILOT M31LRN 2015 and conclude that it cannot be explained by the onset of a common envelope evolution (CEE). Instead we conjecture that a $M \simeq 0.5 – 1 ~M_\odot$ main sequence star accreted $0.05 ~M_\odot$ from the giant star, possibly during a periastron passage. The main sequence star accreted mass through an accretion disc, that launches jets. The radiation from the disk and the collision of the jets with the ambient gas can account for the luminosity of the event. Along similar lines, we suggest that the 2013 eruption of SNHunt 275 can also be explained by the High-Accretion-Powered ILOT (HAPI) model. In this case a massive secondary star $M_2 \gtrsim 10 ~M_\odot$ accreted $\approx 0.05 ~M_\odot$ from a much more massive and more evolved star during a periastron passage. If the much more energetic 2015 outburst of SNHunt 275 was not a supernova explosion, it might have been a full merger event, or else can be accounted for by a the HAPI-jets model in a very highly eccentric orbit.
N. Soker and A. Kashi
Wed, 25 May 16
14/62
Comments: Submitted. Comments welcome
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