Mon. Not. R. Astron. Soc., 458, 950-962 (2016/May-1)
Massive star mergers and the recent transient in NGC 4490: a more massive cousin of V838 Mon and V1309 Sco.
SMITH N., ANDREWS J.E., VAN DYK S.D., MAUERHAN J.C., KASLIWAL M.M., BOND H.E., FILIPPENKO A.V., CLUBB K.I., GRAHAM M.L., PERLEY D.A., JENCSON J., BALLY J., UBEDA L. and SABBI E.
Abstract (from CDS):
The Galactic transient V1309 Sco was the result of a merger in a low-mass star system, while V838 Mon was thought to be a similar merger event from a more massive B-type progenitor. In this paper, we study a recent optical and infrared (IR) transient discovered in the nearby galaxy NGC 4490 named NGC 4490-OT2011 (NGC 4490-OT hereafter), which appeared similar to these merger events (unobscured progenitor, irregular multi-peaked light curve, increasingly red colour, similar optical spectrum, IR excess at late times), but which had a higher peak luminosity and longer duration in outburst. NGC 4490-OT has less in common with the class of SN 2008S-like transients. A progenitor detected in pre-eruption Hubble Space Telescope (HST) images, combined with upper limits in the IR, requires a luminous and blue progenitor that has faded in late-time HST images. The same source was detected by Spitzer and ground-based data as a luminous IR (2-5 µm) transient, indicating a transition to a self-obscured state qualitatively similar to the evolution seen in other stellar mergers and in luminous blue variables. The post-outburst dust-obscured source is too luminous and too warm at late times to be explained with an IR echo, suggesting that the object survived the event. The luminosity of the enshrouded IR source is similar to that of the progenitor. Compared to proposed merger events, the more massive progenitor of NGC 4490-OT seems to extend a correlation between stellar mass and peak luminosity, and may suggest that both of these correlate with duration. We show that spectra of NGC 4490-OT and V838 Mon also resemble light-echo spectra of η Car, prompting us to speculate that η Car may be an extreme extension of this phenomenon.
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
binaries: general - circumstellar matter - stars: evolution - stars: massive - stars: winds, outflows
NAME NGC 4490-OT2011 N=1.
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