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Published in 2020 at "Acta Astronautica"
DOI: 10.1016/j.actaastro.2020.02.052
Abstract: Abstract Increasing interest in asteroid mining and in-situ resource utilization will lead to an increase in asteroid surface operations. The geophysical properties of asteroids are often unknown and play a significant role in the resulting…
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Keywords:
spacecraft trajectory;
splitting contact;
asteroid;
contact ... See more keywords
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Published in 2020 at "Icarus"
DOI: 10.1016/j.icarus.2019.113602
Abstract: Abstract Over the last couple decades, numerous papers based on lightcurve observations of asteroids have derived shapes that were claimed to represent “contact binary” or fluid equilibrium figures. From these shapes, the authors then presumed…
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Keywords:
binary brick;
analysis;
asteroid lightcurves;
tell contact ... See more keywords
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Published in 2017 at "New Astronomy"
DOI: 10.1016/j.newast.2017.04.008
Abstract: Abstract 07g-3-00820 is a K-type contact binary system with a period of 0.2269551 days. This extremely short period makes this system a rare target whose period is close to the empirical limit (0.22 days). Rc…
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Keywords:
photometric study;
system;
07g 00820;
period ... See more keywords
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Published in 2017 at "New Astronomy"
DOI: 10.1016/j.newast.2017.06.006
Abstract: Abstract We present the first CCD sets of complete light curves for the W Ursae Majoris system NSVS 1557555. The observations were performed in the B, V and I c bands using the 0.25 m…
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Keywords:
system;
solution;
type;
nsvs 1557555 ... See more keywords
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Published in 2019 at "New Astronomy"
DOI: 10.1016/j.newast.2019.04.007
Abstract: Abstract AST3-1 is the second-generation optical photometric telescope at Dome A in Antarctica. In this study, photometric solutions of three eclipsing binaries comprising AST19571, AST21541, and AST38503 were determined for the first time using the…
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Keywords:
ast21541 ast38503;
eclipsing binaries;
ast19571 ast21541;
contact binary ... See more keywords
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Published in 2017 at "Publications of the Astronomical Society of the Pacific"
DOI: 10.1088/1538-3873/aa8bb0
Abstract: V2284 Cyg is a neglected W UMa-type binary star for photometric investigations. Monitored by the Kepler Space Telescope from 2009 to 2013, its light curves are continuously stable, suggesting that both components are inactive during…
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Keywords:
cyg;
substellar object;
contact binary;
v2284 cyg ... See more keywords
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Published in 2020 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/20/1/10
Abstract: Multi-color light curves of V1197 Her were obtained with the 2.4 meter optical telescope at Thai National Observatory and the Wilson-Devinney (W-D) program is used to model the observational light curves. The photometric solutions reveal…
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Keywords:
primary star;
star;
contact;
odot odot ... See more keywords
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Published in 2023 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/acd73c
Abstract: We presented the first photometric and orbital period investigations for a neglected total-eclipse contact binary IP Lyn. The photometric solutions derived from both ground-based and several surveys' observations suggested that it is a shallow contact…
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Keywords:
contact;
contact binary;
mass ratio;
mass ... See more keywords
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Published in 2017 at "Astronomy Reports"
DOI: 10.1134/s106377291712006x
Abstract: The results of three-dimensional numerical simulations of the gaseous envelope of a contact binary star with parameters similar to those of SV Cen are presented. The outflow of matter from the vicinity of the Lagrange…
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Keywords:
gas dynamical;
binary stars;
dynamical features;
envelopes contact ... See more keywords