Results 71 to 80 of about 19,129 (209)
Modelling of W UMa-type variable stars
W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand how these systems form and evolve requires observations spanning many years, followed by detailed models of as many of them as possible.
P. Skelton, D. Smits
doaj
The Long-period Spectroscopic Orbit and Dust Creation in the Wolf–Rayet Binary System WR 125
Several long-period binaries with a carbon-rich Wolf–Rayet star and an OB star produce dust in their wind collisions. In eccentric binaries, this is seen most strongly near periastron passage.
Noel D. Richardson +10 more
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Rotational properties of hypermassive neutron stars from binary mergers [PDF]
Matthias Hanauske +6 more
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Data Release 3 (DR3) from the Gaia Mission includes radial velocity measurements of over 33 million targets. Among many scientific applications, the overlap of this stellar sample with targeted exoplanet transit survey stars presents an opportunity to ...
Quadry Chance +5 more
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Strange Quark Stars in Binaries: Formation Rates, Mergers, and Explosive Phenomena [PDF]
Grzegorz Wiktorowicz +3 more
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The X-Ray Emission Reveals the Coronal Activities of Semi-detached Binaries
X-ray emission is an important tracer of stellar magnetic activity. We carried out a systematic correlation analysis for the X-ray luminosity $\mathrm{log}{L}_{{\rm{X}}}$ , bolometric luminosity $\mathrm{log}{L}_{\mathrm{bol}}$ , and X-ray activity ...
Junhui Liu, Jianfeng Wu
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Observational studies of early-type binary stars: VV Orionis [PDF]
D. Terrell, U. Munari, A. Siviero
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Many stars exist in binary or multiple systems where tidal interactions modify rotational evolution. In single stars, Many stars, including those in binary or multiple systems, exhibit modified rotational evolution due to tidal interactions.
Ilay Kamai, Hagai B. Perets
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A survey of eclipsing binary stars in the eastern spiral arm of M31 [PDF]
I. Todd +5 more
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