Results 291 to 300 of about 209,402 (313)

A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]. [PDF]

Nat Astron
Zavala JA, Castellano M, Akins HB, Bakx TJLC, Burgarella D, Casey CM, Chávez Ortiz ÓA, Dickinson M, Finkelstein SL, Mitsuhashi I, Nakajima K, Pérez-González PG, Arrabal Haro P, Bergamini P, Buat V, Backhaus B, Calabrò A, Cleri NJ, Fernández-Arenas D, Fontana A, Franco M, Grillo C, Giavalisco M, Grogin NA, Hathi N, Hirschmann M, Ikeda R, Jung I, Kartaltepe JS, Koekemoer AM, Larson RL, McKinney J, Papovich C, Rosati P, Saito T, Santini P, Terlevich R, Terlevich E, Treu T, Yung LYA.   +39 more
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Improving patient clustering by incorporating structured variable label relationships in similarity measures. [PDF]

BMC Med Res Methodol
Lambert J, Leutenegger AL, Baudot A, Jannot AS.   +3 more
europepmc   +1 more source

Enhancing market trend prediction using convolutional neural networks on Japanese candlestick patterns. [PDF]

PeerJ Comput Sci
Mersal ER, Karaoğlan KM, Kutucu H.
europepmc   +1 more source

Light curve analysis and evolutionary status of four newly identified short-period eclipsing binaries. [PDF]

Sci Rep
Darwish MS, Abdelkawy AGA, Hamed GM.
europepmc   +1 more source

LONEStar: The Lunar Flashlight Optical Navigation Experiment. [PDF]

J Astronaut Sci
Krause M, Thrasher A, Soni P, Smego L, Isaac R, Nolan J, Pledger M, Lightsey EG, Ready WJ, Christian J.   +9 more
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Be Stars in Binaries

Astrophysics and Space Science, 2005
A brief review of Be stars in binaries is presented. Attention is paid to systems, where the Be phenomenon is clearly connected to the duplicity, but is not a simple consequence of mass transfer.
openaire   +2 more sources

Binary Stars

Science, 1984
Most stars in the solar neighborhood are either double or multiple systems. They provide a unique opportunity to measure stellar masses and radii and to study many interesting and important phenomena. The best candidates for black holes are compact massive components of two x-ray binaries: Cygnus X-1 and LMC X-3.
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