Results 261 to 270 of about 31,802 (281)

Primordial black holes and their gravitational-wave signatures. [PDF]

Living Rev Relativ
Bagui E, Clesse S, De Luca V, Ezquiaga JM, Franciolini G, García-Bellido J, Joana C, Kumar Jain R, Kuroyanagi S, Musco I, Papanikolaou T, Raccanelli A, Renaux-Petel S, Riotto A, Ruiz Morales E, Scalisi M, Sergijenko O, Ünal C, Vennin V, Wands D, LISA Cosmology Working Group.   +20 more
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Utilizing statistical analysis for motion imagination classification in brain-computer interface systems. [PDF]

PLoS One
Li Y, Zhang J.
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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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Carbon and oxygen isotope evidence for a protoplanetary disk origin of organic solids in meteorites. [PDF]

Proc Natl Acad Sci U S A
Lawrence WM, Blake GA, Eiler J.
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Multi-messenger gravitational lensing. [PDF]

Philos Trans A Math Phys Eng Sci
Smith GP, Baker T, Birrer S, Collins CE, Ezquiaga JM, Goyal S, Hannuksela OA, Hemanta P, Hendry MA, Janquart J, Keitel D, Levan AJ, Lo RKL, More A, Nicholl M, Pastor-Marazuela I, Ponte Pérez AI, Ubach H, Uronen LE, Wright M, Zumalacarregui M, Bianco F, Çalişkan M, Chan JCL, Colangeli E, Gompertz BP, Haines CP, Hayes EE, Hu B, Lamb GP, Liu A, Mandhai S, Narola H, Nguyen QL, Poon JSC, Ryczanowski D, Seo E, Shajib AJ, Shan X, Tanvir N, Vujeva L.   +40 more
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An automatic NGS feature extraction algorithm for predicting EBV-associated nasopharyngeal cancer and high-risk mutation. [PDF]

Virol J
Wang Y, Huang H, Xiao X, Wei J, Long T, Huang C, Ai W, Tong Y, Guo L, Lu R, Gao C.   +10 more
europepmc   +1 more source

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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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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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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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