Results 21 to 30 of about 202,500 (144)
Sculpting the circumbinary planet size distribution through resonant interactions with companion planets [PDF]
, 2022 Resonant locking of two planets is an expected outcome of convergent disc migration. The planets subsequently migrate together as a resonant pair. In the context of circumbinary planets, the disc is truncated internally by the binary.
Evan Fitzmaurice, D. Martin, D. Fabrycky
semanticscholar +1 more source
HD 143006: circumbinary planet or misaligned disc? [PDF]
, 2021 Misalignments within protoplanetary discs are now commonly observed, and features such as shadows in scattered light images indicate departure from a co-planar geometry.
G. Ballabio +5 more
semanticscholar +1 more source
TOI-1338: TESS’ First Transiting Circumbinary Planet [PDF]
Astronomical Journal, 2020 We report the detection of the first circumbinary planet (CBP) found by Transiting Exoplanet Survey Satellite (TESS). The target, a known eclipsing binary, was observed in sectors 1 through 12 at 30 minute cadence and in sectors 4 through 12 at 2 minute ...
V. Kostov +67 more
semanticscholar +1 more source
BEBOP III. Observations and an independent mass measurement of Kepler-16 (AB) b -- the first circumbinary planet detected with radial velocities [PDF]
, 2021 The radial velocity method is amongst the most robust and most established means of detecting exoplanets. Yet, it has so far failed to detect circumbinary planets despite their relatively high occurrence rates.
A. Triaud +32 more
semanticscholar +1 more source
Follow‐up observations of the binary system γ Cep
Astronomische Nachrichten, Volume 343, Issue 5, June 2022., 2022 Abstract We present follow‐up imaging and spectroscopic observations of the exoplanet host star γ Cep A, and of its low‐mass stellar companion γ Cep B. We used the lucky‐imager AstraLux at the Calar Alto observatory to follow the orbital motion of the companion around its primary, whose radial velocity (RV) was determined with spectra of the star ...
Markus Mugrauer +4 more
wiley +1 more source
Planet migration in massive circumbinary discs [PDF]
Monthly notices of the Royal Astronomical Society, 2023 Most stars are in multiple systems, with the majority of those being binaries. A large number of planets have been confirmed in binary stars and therefore it is important to understand their formation and dynamical evolution.
Matthew Teasdale, D. Stamatellos
semanticscholar +1 more source
Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary [PDF]
Astronomical Journal, 2020 We report the discovery of a Neptune-sized ( ) transiting circumbinary planet, Kepler-1661 b, found in the Kepler photometry. The planet has a period of ∼175 days and its orbit precesses with a period of only 35 yr. The precession causes the alignment of
Q. Socia +9 more
semanticscholar +1 more source
Creep Tide Model for the 3-Body Problem. The rotational evolution of a circumbinary planet [PDF]
, 2021 We present a tidal model for treating the rotational evolution in the general three-body problem with arbitrary viscosities, in which all the masses are considered to be extended and all the tidal interactions between pairs are taken into account.
F. Zoppetti +3 more
semanticscholar +1 more source
The Astrophysical Journal, 2023 Some evolved binaries, namely post–asymptotic giant branch (AGB) binaries, are surrounded by stable and massive circumbinary disks similar to protoplanetary disks found around young stars. Around 10% of these disks are transition disks: they have a large
Narsireddy Anugu +19 more
doaj +1 more source
The EBLM project – VII. Spin–orbit alignment for the circumbinary planet host EBLM J0608-59 A/TOI-1338 A [PDF]
Monthly notices of the Royal Astronomical Society, 2020 A dozen short-period detached binaries are known to host transiting circumbinary planets. In all circumbinary systems so far, the planetary and binary orbits are aligned within a couple of degrees.
Vedad Kunovac Hodžić +16 more
semanticscholar +1 more source