Results 341 to 350 of about 303,706 (359)

A steady-state MR fingerprinting sequence optimization framework applied to the fast 3D quantification of fat fraction and water T1 in the thigh muscles. [PDF]

Magn Reson Med
Slioussarenko C, Baudin PY, Marty B.
europepmc   +1 more source

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
europepmc   +1 more source

A small and vigorous black hole in the early Universe. [PDF]

Nature
Maiolino R, Scholtz J, Witstok J, Carniani S, D'Eugenio F, de Graaff A, Übler H, Tacchella S, Curtis-Lake E, Arribas S, Bunker A, Charlot S, Chevallard J, Curti M, Looser TJ, Maseda MV, Rawle TD, Rodríguez Del Pino B, Willott CJ, Egami E, Eisenstein DJ, Hainline KN, Robertson B, Williams CC, Willmer CNA, Baker WM, Boyett K, DeCoursey C, Fabian AC, Helton JM, Ji Z, Jones GC, Kumari N, Laporte N, Nelson EJ, Perna M, Sandles L, Shivaei I, Sun F.   +38 more
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Spectroscopic binary stars and the CHARA array

SPIE Proceedings, 2003
Georgia State University's Center for High Angular Resolution Astronomy (CHARA) operates a multi-telescope, long-baseline, optical/infrared interferometric array on Mt. Wilson, California. Since its inception, one of the primary scientific goals for the CHARA Array has been the resolution of spectroscopic binary stars, which offer tremendous potential ...
T. ten Brummelaar, Nils H. Turner, Thomas Fallon, Chad Ogden, A. Jerkstrand, Stephen T. Ridgway, S. F. Taylor, Harold A. McAlister, Laszlo Sturmann, J. Seymour, William G. Bagnuolo, D. H. Berger, Judit Sturmann   +12 more
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Study of physical properties of spectroscopic binary stars

Astrophysics and Space Science, 1982
The main results of a study of a catalogue of physical parameters of 1041 spectroscopic binaries are presented. The distribution of spectroscopic binaries over all main parametersM1, a, e, M1/M2, P, and certain dependencies between some of them have been found.
L. R. Yungelson, E. I. Popova, Alexander V. Tutukov   +2 more
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The mass-ratio distribution of spectroscopic binary stars

Astrophysics and Space Science, 1992
In order to determine the mass-ratio distribution of spectroscopic binary stars, the selection effects that govern the observations of this class of binary systems are investigated. The selection effects are modelled numerically and analytically. The results of the models are compared to the data inThe Eighth Catalogue of the Orbital Elements of ...
S. J. Hogeveen
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Spectroscopic Binary Stars

Publications of the Astronomical Society of the Pacific, 1898
R. Aitken
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Forty-two Spectroscopic Binary Stars

Publications of the Astronomical Society of the Pacific, 1930
F. Neubauer
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Three new spectroscopic binary stars.

Publications of the Astronomical Society of the Pacific, 1999
W. W. Campbell
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Spectroscopic Binary Stars

2004
A. Batten
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