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The planets around the post-common envelope binary NN Serpentis

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Hessman, Frederic V., Beuermann, K., Dreizler, S., Marsh, T. R., Parsons, S. G., Copperwheat, C. M., Winget, Donald Earl, Miller, G. F., Hermes, J. J., Schreiber, Matthias R., Kley, W., Dhillon, V. S. and Littlefair, S. P. (2011) The planets around the post-common envelope binary NN Serpentis. In: Planetary Systems Beyond the Main Sequence. Published in: AIP Conference Proceedings, Vol.1331 (No.1). pp. 281-286. doi:10.1063/1.3556212 ISSN 0094-243X.

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Official URL: http://dx.doi.org/10.1063/1.3556212

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Abstract

We have detected 2 circumbinary planets around the close binary system NN Serpentis using the orbital time delay effect measured via the sharp eclipses of the white dwarf primary. The present pre-cataclysmic binary was formed when the original ~2 M primary expanded into a red giant, causing the secondary star to drop from its original orbit at a separation of about 1.4 A.U. down to its current separation at 0.0043 A.U. A quasi-adiabatic evolution of the circumbinary planets' orbits during the common-envelope phase would have placed them in unstable configurations, suggesting that they may have suffered significant orbital drag effects and were originally in much larger orbits. Alternatively, they may have been created as 2nd-generation planets during the last million years from the substantial amount of material lost during the creation of the binary, making them the youngest planets known. Either solution shows how little we actually understand about planetary formation. ©2011 American Institute of Physics

Item Type: Conference Item (Paper)
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Library of Congress Subject Headings (LCSH): Eclipses, White dwarf stars, Extrasolar planets, Stellar winds
Journal or Publication Title: AIP Conference Proceedings
Publisher: American Institute of Physics
ISSN: 0094-243X
Official Date: 10 March 2011
Dates:
DateEvent
10 March 2011Published
Volume: Vol.1331
Number: No.1
Page Range: pp. 281-286
DOI: 10.1063/1.3556212
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Conference Paper Type: Paper
Title of Event: Planetary Systems Beyond the Main Sequence
Type of Event: Conference
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