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|Title:||Infrared observations of the recurrent nova T Pyxidis: ancient dust basks in the warm glow of the 2011 outburst|
Gehrz, R. D.
Helton, L. A.
Bode, M. F.
Osborne, J. P.
Banerjee, D. P. K.
Walter, F. M.
Woodward, C. E.
Eyres, S. P. S.
Oliveira, J. M.
Page, K. L.
Rushton, M. T.
|Citation:||Monthly Notices of the Royal Astronomical Society , 2012, 424 (1), pp. L69-L73|
|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 optical-infrared 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.|
|Rights:||This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2012 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
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