Evidence for the merger hypothesis in V4332 Sgr: a low $^{12}$C/$^{13}$C ratio and multiple outbursts
D. P. K. Banerjee (Physical Research Laboratory, Ahmedabad, India), A. Evans (Keele University, UK), Watson P. Varricatt (UKIRT Observatory), N. M. Ashok (PRL, Ahmedabad, India)

TL;DR
This paper provides evidence that V4332 Sgr was a stellar merger, based on a low $^{12}$C/$^{13}$C ratio and multiple outbursts, supporting the merger hypothesis for luminous red novae.
Contribution
It presents the first direct evidence of a merger in V4332 Sgr through high-resolution infrared spectroscopy revealing a low $^{12}$C/$^{13}$C ratio.
Findings
Low $^{12}$C/$^{13}$C ratio of 3.5±1 indicating deep stellar processing.
Detection of multiple outbursts in V4332 Sgr.
Evidence supporting a merger scenario involving a common envelope.
Abstract
Following the detections of the first extragalactic ``Luminous Red Nova'' (LRN) M31 RV in 1989, and its first Galactic counterpart V4332~Sgr in 1994, there have been many discoveries of similar, or closely related, objects. They are important because they bridge the luminosity gap between the brightest novae and supernovae, a largely unexplored parameter space. The cause of eruptions in LRNe is still unclear, a stellar merger being the most favored mechanism. However, barring V1309~Sco, there has been no direct evidence for a merger in the other objects. Here we present strong evidence that V4332~Sgr was a merger event. High resolution infrared observations of the CO fundamental band show an unusually small C/C ratio of . This indicates that a violent event had occurred, whose effects penetrated deep enough to allow CNO cycle processed C in the inner H…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysical Phenomena and Observations · Astronomy and Astrophysical Research
