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Paper detail

Infrared observations of the recurrent nova T Pyxidis: ancient dust basks in the warm glow of the 2011 outburst

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.

preprint2012arXivOpen access
A. EvansR. D. GehrzL. A. HeltonS. StarrfieldM. F. BodeJ. P. OsborneD. P. K. BanerjeeJ. -U. NessF. M. WalterC. E. WoodwardE. KuulkersS. P. S. EyresJ. M. OliveiraN. M. AshokJ. KrautterT. J. O'BrienK. L. PageM. T. Rushton
astro-ph.SR
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A. EvansR. D. GehrzL. A. HeltonS. StarrfieldM. F. BodeJ. P. OsborneD. P. K. BanerjeeJ. -U. NessF. M. WalterC. E. WoodwardE. KuulkersS. P. S. EyresJ. M. OliveiraN. M. AshokJ. KrautterT. J. O'BrienK. L. PageM. T. Rushton

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