Results 221 to 230 of about 3,234,913 (246)

Shock compression of FeOOH and implications for iron-water interactions in super-earth magma oceans. [PDF]

Nat Commun
Zhang Y, Bali K, Dorn C, Ravasio A, Yang H, Pandolfi S, Chen AJ, Wei X, Libon L, Che Q, Zheng D, Boulard E, Benuzzi-Mounaix A, Lee HJ, Galtier E, Czapla NA, Sokaras D, Alonso-Mori R, Gleason AE, Shim SH, Morard G, Mao WL.   +21 more
europepmc   +1 more source

Beyond intracranial pressure: Cerebrospinal fluid compartmentalization in spaceflight‐associated neuro‐ocular syndrome

Experimental Physiology, Volume 111, Issue 9, Page 3916-3918, 1 September 2026.
Susan P. Mollan, Damian M. Bailey
wiley   +1 more source

Preparation of Low-Surface-Energy SSBR@FA Hybrid Fillers via Solution Mechanochemical Approach and Its Enhancement in Mechanical Strength on the Modified FA/SBR Composites. [PDF]

Polymers (Basel)
Gao W, Zhao J, Qi W, Huang Z, Liu G, Feng C, Sang C, Wang X, Zhang X.   +8 more
europepmc   +1 more source

The Infrared Spectrum of Uranus Revealed with JWST

Roman M, Fletcher L, Hammel H, King O, Irwin P, de Pater I, Moses J, Orton G, Rowe-Gurney N, Melin H, Hedman M, Toogood S, Harkett J, Penn J, Milam S.   +14 more
europepmc   +1 more source

Zircon behavior in the partially melted planetary mantle

Yakimenko A, Borisova A, Fedortchouk Y, Fairhurst L.   +3 more
europepmc   +1 more source

Disk evaporation in a planetary nebula

Astronomy and Astrophysics, 2010
Aims.Binary interactions are believed to be important contributors to the structures seen in planetary nebulae (PN), and the sole cause of the newly discovered compact dust disks.
Marcin Hajduk, Eric Lagadec, Albert Zijlstra   +2 more
exaly   +2 more sources

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N-body interactions in proto-planetary disks: A study of collision velocities and impact angles

2023
We show the distribution of collision parameters of planetesimals and planetary embryos in an evolving protoplanetary disk for various binary star–giant planet configurations. This statistical study provides an overview which and how many of the mutual disk object collisions have to be studied in more detail with SPH (smooth particle ...
Maximilian Zimmermann, Elke Pilat-Lohinger   +1 more
openaire   +2 more sources

The HR 8799 debris disk: Shaped by planetary migration and a possible fifth outermost planet

Astronomy and Astrophysics
International audienceContext. The HR 8799 system hosts four giant planets between a warm and cold debris disk and has an extended dusty tail beyond. It serves as an ideal laboratory for studying planetary formation and evolution.
Tim Pearce, Pedro Poblete, Carolina Charalambous   +2 more
exaly   +2 more sources

Excitation of Planetary Obliquities through Planet–Disk Interactions [PDF]

Astrophysical Journal, 2019
The tilt of a planet's spin axis off its orbital axis ("obliquity") is a basic physical characteristic that plays a central role in determining the planet's global circulation and energy redistribution.
Konstantin Batygin, Sarah Millholland
exaly   +1 more source

Planet-Disk Interactions and Early Evolution of Planetary Systems [PDF]

, 2014
The great diversity of extrasolar planetary systems has challenged our understanding of how planets form, and how their orbits evolve as they form. Among the various processes that may account for this diversity, the gravitational interaction between ...
Clement Baruteau
exaly   +3 more sources