Results 51 to 60 of about 202,500 (144)
The Role of Disc Self-Gravity in Circumbinary Planet Systems: II. Planet Evolution [PDF]
The authors thank the referee for the comments and suggestions in their helpful report. Computer time for the simulations performed with GENESIS was provided by HPC resources of Cines under the allocation A0010406957 made by GENCI (Grand Equipement ...
M. Mutter, A. Pierens, R. Nelson
semanticscholar +1 more source
Orbital dynamics of two circumbinary planets around misaligned eccentric binaries [PDF]
Cheng Chen +2 more
openalex +1 more source
Empirical Stability Criteria for 3D Hierarchical Triple Systems. I. Circumbinary Planets
In this work we revisit the problem of the dynamical stability of hierarchical triple systems with applications to circumbinary planetary orbits. We derive critical semimajor axes based on simulating and analyzing the dynamical behavior of 3 × 10 ^8 ...
Nikolaos Georgakarakos +3 more
doaj +1 more source
The Influence of Tight Binaries on Protoplanetary Disk Masses
Binary systems are a common site of planet formation, despite the destructive effects of the binary on the disk. While surveys of planet-forming material have found diminished disk masses around binaries with medium separation (∼10–100 au), less is known
Kevin Flaherty +7 more
doaj +1 more source
We present an analysis of eclipse timing variations in Kepler-451 using data spanning 2004–2024 from both ground- and space-based observations. Using two data sets, Data Set A (DS-A) and Data Set B (DS-B), we constructed updated O–C diagrams. By modeling
Huseyin Er +7 more
doaj +1 more source
Planetary Rhythms: Synchronous Circulation on Variably Irradiated Asynchronous Planets
Tidal locking of planets to their host stars results in an atmospheric circulation with a hotspot fixed to the frame of reference of the planet. On the other hand, asynchronously rotating planets feature moving hotspots either lagging or leading the ...
Deepayan Banik
doaj +1 more source
Circumbinary planet study around NSVS 14256825
The period variability of (O-C) diagram of an eclipsing binary, NSVS 14256825, which is composed of a hot subdwarf type OB star (sdOB) and a main-sequence low-mass type M star (dM) in close orbit with period P=0.110374 days, previously showed sinusoidal ...
P. Sappankum +6 more
semanticscholar +1 more source
Close binary systems present challenges to planet formation. As binary separations decrease, so do the occurrence rates of protoplanetary disks in young systems and planets in mature systems.
Benjamin M. Tofflemire +10 more
doaj +1 more source
Searching for Small Circumbinary Planets. I. The STANLEY Automated Algorithm and No New Planets in Existing Systems [PDF]
David V. Martin +3 more
openalex +1 more source
Stable climates for temperate rocky circumbinary planets [PDF]
Thaddeus D. Komacek
openalex +2 more sources

