Results 31 to 40 of about 3,219 (118)

Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars

The Astronomical Journal
Transiting giant planets provide a natural opportunity to examine stellar obliquities, which offer clues about the origin and dynamical histories of close-in planets.
Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Erik Petigura, Vighnesh Nagpal, Sarah Blunt   +5 more
doaj   +1 more source

Comprehensive Surrogate Models for Predicting the Melt Conveying Characteristics of Channel Segments in High‐Performance Single‐Screw Extruders

Polymer Engineering &Science, EarlyView.
Generalized analytical equations were developed that accurately predict the local pumping characteristics, viscous dissipation, and average shear rates in channels of both conventional and high‐performance single‐screw extruders. Applied within segmented extruder calculations, these models aid in screw design and process troubleshooting without the ...
Daniel Herzog, Wolfgang Roland, Christian Marschik, Gerald Berger‐Weber   +3 more
wiley   +1 more source

On the Abundance of Circumbinary Planets

, 2014
We present here the first observationally based determination of the rate of occurrence of circumbinary planets. This is derived from the publicly available Kepler data, using an automated search algorithm and debiasing process to produce occurrence ...
Armstrong, D. J., Brown, D., Chew, Y. Gómez Maqueo, Faedi, F., Martin, D., Osborn, H., Pollacco, D., Udry, S.   +7 more
core   +1 more source

Time variation of Kepler transits induced by stellar rotating spots - a way to distinguish between prograde and retrograde motion I. Theory [PDF]

, 2015
Some transiting planets discovered by the Kepler mission display transit timing variations (TTVs) induced by stellar spots that rotate on the visible hemisphere of their parent stars.
Holczer, Tomer, Mazeh, Tsevi, Shporer, Avi   +2 more
core   +2 more sources

Synthesis of Large‐Area 2D Prussian Blue as Ion‐Transport Channels for Non‐Volatile Memristors

Small, EarlyView.
A robust liquid‐liquid interfacial synthesis enables continuous, large‐area 2D Prussian blue films with tunable thickness from ∼2 nm to hundreds of nanometers. Controlled reduction guides slow, directional layer growth, yielding high‐quality flakes. These films show exceptional ion transport and device integration, demonstrated in memristors with long ...
Ramón Torres‐Cavanillas, Hewen Chen, Javier Castells‐Gil, Dunia Hidalgo, Maria Arenós‐Amat, Christopher S. Allen, Gianluca fabi, Georg Gramse, Eugenio Coronado, Lapo Bogani   +9 more
wiley   +1 more source

Constraints on the habitability of extrasolar moons [PDF]

, 2012
Detections of massive extrasolar moons are shown feasible with the Kepler space telescope. Kepler's findings of about 50 exoplanets in the stellar habitable zone naturally make us wonder about the habitability of their hypothetical moons.
Barnes, Rory, Heller, René
core   +1 more source

The light-curve intrinsic variability in 47 Kepler contact binary stars [PDF]

, 2022
B. Dȩbski
openalex   +1 more source

Aligning Real‐Time Recurrence Computational Fluid Dynamics Simulations with Plant Data for the Ruhrstahl–Heraeus Degassing Process of Steel

steel research international, EarlyView.
Uncertainties exist in computational fluid dynamics (CFD) modeling of complex metallurgical processes, even when partly validated by laboratory experiments. rCFD enables computationally efficient prediction of long‐term RH degassing and can be adapted to vary flow conditions.
Xiaomeng Zhang, Maria Thumfart, Roman Rössler, Stefan Pirker   +3 more
wiley   +1 more source

Transit Timing and Duration Variations for the Discovery and Characterization of Exoplanets

, 2017
Transiting exoplanets in multi-planet systems have non-Keplerian orbits which can cause the times and durations of transits to vary. The theory and observations of transit timing variations (TTV) and transit duration variations (TDV) are reviewed.
A Pál, A Wolszczan, AR Dobrovolskis, BT Montet, BT Montet, C Beichman, C Sterken, C Wilson, D Jontof-Hutter, D Nesvorný, D Nesvorný, D Nesvorný, D Nesvorný, D Nesvorný, D Nesvorný, D Nesvorný, D Ragozzine, DM Kipping, DV Martin, E Agol, E Agol, EJ Lee, EM Price, G Laughlin, GM Szabó, GR Ricker, H Rauer, J Eastman, J Miralda-Escudé, J Schneider, JA Carter, JA Carter, JA Carter, JC Adams, JC Becker, JH Steffen, JH Steffen, JH Steffen, JJ Lissauer, JM Almenara, JM Almenara, JS Heyl, JW Barnes, JW Xie, K Masuda, KM Deck, KM Deck, LR Doyle, M Gillon, M Oshagh, MJ Holman, MJ Holman, NP Gibson, P Ioannidis, P Mayer, RI Dawson, RK Ulrich, S Ginzburg, S Hadden, S Hadden, S Hadden, S Meschiari, S Seager, SCC Barros, SM Mills, SM Mills, SM Mills, T Borkovits, UJ Verrier Le, VB Kostov, VB Kostov, WD Cochran, WF Welsh, Y Lithwick   +73 more
core   +1 more source

Planet Formation in Circumbinary Configurations: Turbulence Inhibits Planetesimal Accretion [PDF]

, 2012
The existence of planets born in environments highly perturbed by a stellar companion represents a major challenge to the paradigm of planet formation.
Meschiari, Stefano
core   +2 more sources