The Infrared Evolution of Dust in V838 Monocerotis C
Draft version August 19, 2021 Typeset using LATEX twocolumn style in AASTeX63 The Infrared Evolution of Dust in V838 Monocerotis C. E. Woodward ,1 A. Evans ,2 D. P. K. Banerjee ,3 T. Liimets ,4, 5 A. A. Djupvik ,6 S. Starrfield ,7 G. C. Clayton ,8 S. P. S. Eyres ,9 R. D. Gehrz ,1 and R. M. Wagner 10, 11 1Minnesota Institute for Astrophysics, University of Minnesota, 116 Church Street SE, Minneapolis, MN 55455, USA 2Astrophysics Group, Keele University, Keele, Staffordshire, ST5 5BG, UK 3Physical Research Laboratory, Navrangpura, Ahmedabad, Gujarat 380009, India 4Astronomick´y´ustav,Akademie vˇed Cesk´erepubliky,ˇ v.v.i., Friˇcova298, 251 65 Ondˇrejov,Czech Republic 5Tartu Observatory, University of Tartu, Observatooriumi 1, 61602 T~oravere, Estonia 6Nordic Optical Telescope, Rambla Jos´eAna Fern´andezP´erez 7, ES-38711 Bre~naBaja, Spain 7School of Earth and Space Exploration, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA 8Louisiana State University, Baton Rouge, Department of Physics & Astronomy Baton Rouge, LA 70803-001, USA 9Faculty of Computing, Engineering & Science, University of South Wales, Pontypridd, CF37 1DL, UK 10Department of Astronomy, The Ohio State University, 140 W. 18th Avenue, Columbus, OH 43210, USA 11Large Binocular Telescope Observatory, 933 North Cherry Avenue, Tucson, AZ 85721, USA (Received 2021 June 21; Accepted 2021 August 17; Published To Appear in The Astronomical Journal) ABSTRACT Luminous Red Variables (LRVs) are most likely eruptions that are the outcome of stellar mergers. V838 Mon is one of the best-studied members of this class, representing an archetype for stellar mergers resulting from B-type stars.
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