Results 31 to 40 of about 374,157 (297)
Classical Observations of Visual Binary and Multiple Stars [PDF]
AbstractChanges in the double star database are highlighted, describing various methods of observation (both historically and those of the past few years) and their effectiveness in different regimes of separation space. The various niches for wide- and narrow-field work as they apply to double and multiple stars are examined and the different types of
Brian D. Mason
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Visual binary stars: data to investigate formation of binaries [PDF]
Statistics of orbital parameters of binary stars as well as statistics of their physical characteristics bear traces of star formation history. However, statistical investigations of binaries are complicated by lacking or incomplete observational data and by a number of observational selection effects.
Dana Kovaleva+3 more
arxiv +3 more sources
Classical Wolf–Rayet (WR) stars are descendants of massive OB-type stars that have lost their hydrogen-rich envelopes and are in the final stages of stellar evolution, possibly exploding as Type Ib/c supernovae.
Amanda Holdsworth+21 more
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Kinematics of Hipparcos Visual Binaries. I. Stars whit Orbital Solutions [PDF]
A. Bartkevičius, A. Gudas
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Mean densities of visual binary stars.
M. A. Giannuzzi, L. Bianco
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Note on the Comparative Eccentricities of Visual and Spectroscopic Binary Stars [PDF]
T. J. J. See
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Graphical determination of orbits of visual binary stars
J. J. Nassau, P. D. Wilkins
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Spectroscopic Orbits of Subsystems in Multiple Stars. IX
New spectroscopic orbits of inner subsystems in 14 hierarchies are determined from long-term monitoring with the optical echelle spectrometer, CHIRON.
Andrei Tokovinin
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We present a method to identify likely visual binaries in Gaia eDR3 that does not rely on parallax or proper motion. This method utilizes the various point-spread function sizes of Two Micron All Sky Survey (2MASS)/Gaia, where at
Ilija Medan, Sébastien Lépine
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Abstract Background and purpose For postoperative breast cancer patients, deformable image registration (DIR) is challenged due to the large deformations and non‐correspondence caused by tumor resection and clip insertion. To deal with it, three metrics (fiducial‐, region‐, and intensity‐based) were jointly used in DIR algorithm for improved accuracy ...
Xin Xie+6 more
wiley +1 more source