2013A&A...555A.133B


Query : 2013A&A...555A.133B

2013A&A...555A.133B - Astronomy and Astrophysics, volume 555A, 133-133 (2013/7-1)

The quest for companions to post-common envelope binaries. IV. The 2:1 mean-motion resonance of the planets orbiting NN Serpentis.

BEUERMANN K., DREIZLER S. and HESSMAN F.V.

Abstract (from CDS):

We present 69 new mid-eclipse times of the young post-common envelope binary (PCEB) βobject{NNSer}, which was previously suggested to possess two circumbinary planets. We have interpreted the observed eclipse-time variations in terms of the light-travel time effect caused by two planets, exhaustively covering the multi-dimensional parameter space by fits in the two binary and ten orbital parameters. We supplemented the fits by stability calculations for all models with an acceptable χ2. An island of secularly stable 2:1 resonant solutions exists, which coincides with the global χ2 minimum. Our best-fit stable solution yields current orbital periods Po=15.47yr and Pi=7.65yr and eccentricities eo=0.14 and ei=0.22 for the outer and inner planets, respectively. The companions qualify as giant planets, with masses of 7.0MJup and 1.7MJup for the case of orbits coplanar with that of the binary. The two-planet model that starts from the present system parameters has a lifetime greater than 108yr, which significantly exceeds the age of NN Ser of 106yr as a PCEB. The resonance is characterized by libration of the resonant variable Θ1 and circulation of ωio, the difference between the arguments of periapse of the two planets. No stable nonresonant solutions were found, and the possibility of a 5:2 resonance suggested previously by us is now excluded at the 99.3% confidence level.

Abstract Copyright:

Journal keyword(s): binaries: close - binaries: eclipsing - white dwarfs - stars: individual: NN Serpentis - planets and satellites: detection - planets and satellites: dynamical evolution and stability

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 BD-07 3477 HS* 12 44 20.2386233232 -08 40 16.846099536   10.46 10.594 10.895   sdB2VIIHe3 270 1
2 V* QS Vir EB* 13 49 52.0029035208 -13 13 37.000132212 14.27 14.98 14.40 14.37   DA3+dM 128 1
3 HD 128311 BY* 14 36 00.5602765558 +09 44 47.454573266 9.232 8.441 7.446 6.895 6.425 K3V 292 1
4 V* NN Ser CV* 15 52 56.1203524080 +12 54 44.429312196     16.51     DAO1+M4 257 0
5 Kepler-47 EB* 19 41 11.4983203032 +46 55 13.707336288           ~ 146 1
6 V* HU Aqr CV* 21 07 58.1944529400 -05 17 40.557671916   16.198 15.814 14.891   D+M4V 265 1

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2022.12.05-18:39:37

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