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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
  • Keele University
  • University of Minnesota Twin Cities
  • NASA Ames Research Center
  • Arizona State University
  • Liverpool John Moores University
  • University of Leicester
  • Physical Research Laboratory India
  • ESAC
  • University of Central Lancashire
  • Heidelberg University 
  • University of Manchester

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

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.

Original languageEnglish
Pages (from-to)L69-L73
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume424
Issue number1
DOIs
StatePublished - Jul 2012

Keywords

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

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