Infrared observations of the recurrent nova T pyxidis: Ancient dust basks in the warm glow of the 2011 outburs

A. Evans, R. D. Gehrz, L. A. Helton, S. Starrfield, M. F. Bode, J. P. Osborne, D. P K Banerjee, J. U. Ness, F. M. Walter, C. E. Woodward, E. Kuulkers, S. P S Eyres, J. M. Oliveira, N. M. Ashok, J. Krautter, T. J. O'Brien, K. L. Page, M. T. Rushton

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We present Spitzer Space Telescope and Herschel Space Observatory infrared observations of the recurrent nova T Pyx during its 2011 eruption, complemented by ground-base opticalinfrared photometry. We find that the eruption has heated dust in the pre-existing nebulosity associated with T Pyx. This is most likely interstellar dust swept up by T Pyx-either during previous eruptions or by a wind-rather than the accumulation of dust produced during eruptions. © 2012 The Authors, MNRAS 424, L69-L73 Monthly Notices of the Royal Astronomical Society. © 2012 RAS.
    Original languageEnglish
    Pages (from-to)L69-L73
    JournalMonthly Notices of the Royal Astronomical Society: Letters
    Volume424
    Issue number1
    DOIs
    Publication statusPublished - Jul 2012

    Keywords

    • Circumstellar matter
    • Infrared: stars
    • ISM: general
    • Novae, Cataclysmic variables
    • Stars: individual: T Pyx

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