Results 181 to 190 of about 997,063 (252)

Evidence for a polar circumbinary exoplanet orbiting a pair of eclipsing brown dwarfs. [PDF]

Sci Adv
Baycroft TA, Sairam L, Triaud AHMJ, Correia ACM.   +3 more
europepmc   +1 more source

Magnetic activities of two contact binaries in quadruple stellar systems. [PDF]

Sci Rep
Yang Y, Wang S.
europepmc   +1 more source

Reassessment of Kepler's habitable zone Earth-like exoplanets with data-driven null signal templates. [PDF]

Proc Natl Acad Sci U S A
Robnik J, Seljak U.
europepmc   +1 more source

Unsupervised classification of eclipsing binary light curves through k-medoids clustering. [PDF]

J Appl Stat, 2020
Modak S, Chattopadhyay T, Chattopadhyay AK.   +2 more
europepmc   +1 more source

Deep learning exoplanets detection by combining real and synthetic data. [PDF]

PLoS One, 2022
Cuéllar S, Granados P, Fabregas E, Curé M, Vargas H, Dormido-Canto S, Farias G.   +6 more
europepmc   +1 more source

The Benchmark Eclipsing Binary V530 Ori : A Critical Test of Magnetic Evolution Models for Low-Mass Stars

, 2015
We report accurate measurements of the physical properties (mass, radius, temperature) of components of the G+M eclipsing binary V530 On. The M-type secondary shows a larger radius and a cooler temperature than predicted by standard stellar evolution ...
Lacy, Claud H. Sandberg,, Bruntt, Hans,, Torres, Guillermo,, Feiden, Gregory A.,, Pavlovski, Kresimir,, Clausen, Jens Viggo,, Sabby, Jeffrey A.,   +6 more
core  

Precise orbital parameters,masses, and parallax of the subgiant binary system 12 Persei: a combined spectroscopic-interferometric analysis. [PDF]

Sci Rep
Abushattal AA, Widyan H, Dirk M, Al-Wardat MA, Al-Mashaqbeh M, Mendez RA, Dewi DA, Hussein AM, Abu-Alrob EM.   +8 more
europepmc   +1 more source

The first extragalactic ultra-compact X-ray binary: A candidate black hole-white dwarf system. [PDF]

Innovation (Camb)
Ma QQ, Zhang J, Gu WM, Li Z, Weng SS, Bao T.   +5 more
europepmc   +1 more source

The connection between Delta Scuti stars and close binary parameters

, 2011
With recent advances in CCD technology, it has become possible to detect low-amplitude variability in stars. Thus, the number of low-amplitude variables has increased at an exceptional rate over the past decade.
Turner, Garrison H.
core  

A transiting giant planet in orbit around a 0.2-solar-mass host star. [PDF]

Nat Astron
Bryant EM, Jordán A, Hartman JD, Bayliss D, Sedaghati E, Barkaoui K, Chouqar J, Pozuelos FJ, Thorngren DP, Timmermans M, Almenara JM, Chilingarian IV, Collins KA, Gan T, Howell SB, Narita N, Palle E, Rackham BV, Triaud AHMJ, Bakos GÁ, Brahm R, Hobson MJ, Van Eylen V, Amado PJ, Arnold L, Bonfils X, Burdanov A, Cadieux C, Caldwell DA, Casanova V, Charbonneau D, Clark CA, Collins KI, Daylan T, Dransfield G, Demory BO, Ducrot E, Fernández-Rodríguez G, Fukuda I, Fukui A, Gillon M, Gore R, Hooton MJ, Ikuta K, Jehin E, Jenkins JM, Levine AM, Littlefield C, Murgas F, Nguyen K, Parviainen H, Queloz D, Seager S, Sebastian D, Srdoc G, Vanderspek R, Winn JN, de Wit J, Zúñiga-Fernández S.   +58 more
europepmc   +1 more source