The Infrared Evolution of Dust in V838 Monocerotis

C. E. Woodward*, A. Evans, D. P. K. Banerjee, T. Liimets, A. A. Djupvik, S. Starrfield, G. C. Clayton, S. P. S. Eyres, R. D. Gehrz, R. M. Wagner

*Awdur cyfatebol y gwaith hwn

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

12 Wedi eu Llwytho i Lawr (Pure)


Luminous Red Variables 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. As result of the merger event, "nova-like"eruptions occur driving mass loss from the system. As the gas cools considerable circumstellar dust is formed. V838 Mon erupted in 2002 and is undergoing very dynamic changes in its dust composition, geometry, and infrared luminosity providing a real-time laboratory to validate mineralogical condensation sequences in stellar mergers and evolutionary scenarios. We discuss recent NASA Stratospheric Observatory for Infrared Astronomy 5-38 µm observations combined with archival NASA Spitzer spectra that document the temporal evolution of the freshly formed (within the last ?20 yr) circumstellar material in the environs of V838 Mon. Changes in the 10 µm spectral region are strong evidence that we are witnessing a classical dust condensation sequence expected to occur in oxygen-rich environments where alumina formation is followed by that of silicates at the temperature cools.

Iaith wreiddiolSaesneg
Rhif yr erthygl183
Nifer y tudalennau9
CyfnodolynAstronomical Journal
Rhif cyhoeddi5
Dyddiad ar-lein cynnar7 Hyd 2021
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - 1 Tach 2021

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