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Bibliographic Details
Main Authors: Geballe, T. R., Kaminskiy, B. M., Banerjee, D. P. K., Evans, A., Pavlenko, Y., Rushton, M. T., Popescu, M., Eyres, S. P. S.
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2507.13151
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Table of Contents:
  • We report medium-resolution $0.85-2.45\,μ$m spectroscopy obtained in 2015 and 2022 and high resolution $2.27-2.39\,μ$m and $4.59-4.77\,μ$m spectroscopy obtained in 2015 of V838 Monocerotis, along with modeling of the $0.85-2.45\,μ$ spectrum. V838 Mon underwent a series of eruptions and extreme brightenings in 2002, which are thought to have occured as a result of a stellar merger. The new spectra and modelling of them reveal a disturbed red giant photosphere that is probably continuing to contract and ejecta that are cooling and continuing to disperse at velocities up to 200kms$^{-1}$.