Results 231 to 240 of about 892 (259)

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
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A scalable equivariant graph network framework for precise protein function prediction. [PDF]

Genome Biol
Ran Z, Guo X, Pan T, Bi Y, Hao Y, Sun H, Song J, Li F.   +7 more
europepmc   +1 more source

Machine-learning design of ductile FeNiCoAlTa alloys with high strength. [PDF]

Nature
Sohail Y, Zhang C, Xue D, Zhang J, Zhang D, Gao S, Yang Y, Fan X, Zhang H, Liu G, Sun J, Ma E.   +11 more
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Efficient Approximation with Space Filling Quadtrees: Application to Phase Equilibria in Binary Mixtures. [PDF]

Ind Eng Chem Res
Bell IH.
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Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

Living Rev Sol Phys
Veronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A.   +12 more
europepmc   +1 more source

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Common envelopes in binary star evolution

Publications of the Astronomical Society of the Pacific, 1993
The characteristics of many close, evolved binaries can be understood most easily if there exists some agency that can abstract angular momentum or mass, or both, from the precursor system. Close binaries may be defined as systems in which at least one of the components has filled or will fill its Roche lobe and attempt to transfer matter to its ...
Icko, Jr. Iben, Mario Livio
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Common Envelope Evolution of Massive Binary Stars

Annual Review of Astronomy and Astrophysics, 2000
▪ Abstract  The common envelope phase of binary star evolution plays an essential role in the formation of short period systems containing a compact object. In this process, significant mass and angular momentum are lost, transforming a wide progenitor system into a close remnant binary. The pathways leading to this phase and the outcomes are described.
Ronald E. Taam, Eric L. Sandquist
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AGB stars in binaries and the common envelope interaction

Proceedings of the International Astronomical Union, 2018
AbstractOne may argue that, today, proceedings articles are not useful. Results belong in refereed papers and even reviews are best in publications that are long enough to do justice to the topic reviewed. In this short review, reflecting a presentation that was given at the IAU343 symposium, Why Galaxies Care about AGB Stars, I have therefore ...
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The Formation of Common-Envelope, Pre-Main-Sequence Binary Stars

1999
Recent observational investigations of the frequency of occurrence of premain-sequence binary stars have reinforced earlier suspicions that “binary formation is the primary branch of the star-formation process” (Mathieu 1994). As Bodenheimer et al. (1993) have reviewed, a number of different theories have been proposed to explain the preponderance of ...
J. E. Tohline, J. E. Cazes, H. S. Cohl
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Colorectal cancer statistics, 2023

Ca-A Cancer Journal for Clinicians, 2023
Rebecca L Siegel, Nikita Sandeep Wagle, Robert A Smith   +2 more
exaly