Results 51 to 60 of about 19,129 (209)
Discovery of eclipsing binary central stars in the planetary nebulae M 3-16, H 2-29, and M 2-19 [PDF]
B. Miszalski +4 more
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Abstract:Ultraviolet and X-ray surveys of the W Ursae Majoris type stars are reviewed. These systems exhibit extended coronas and transition regions that are confined close to the optically determined surfaces. Correlations of X-ray activity with period or rotational velocity indicate a turn-over or saturation of emission at the short periods or high ...
openaire +1 more source
Wind accretion in binary stars - I. Mass accretion ratio [PDF]
T. Nagae +5 more
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Modelling the expected very high energy gamma-ray emission from accreting neutron stars in X-ray binaries [PDF]
L. Ducci +3 more
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We present archival Hubble Space Telescope (HST) and JWST ultraviolet through near-infrared time series photometric observations of a massive minimal-contact binary candidate in the metal-poor galaxy Wolf–Lundmark–Melotte ( Z = 0.14 Z _⊙ ).
Maude Gull +17 more
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Astronomical Data Resources for Binary and Multiple Stars
Binary stars form a significant part of stellar population. They are registered and observed by a number of methods. This is the reason for variety of present-day resources of astronomical data dealing with binaries and multiples.
Kovaleva D.
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Short-period Heartbeat Binaries from TESS Full-frame Images
We identify 240 short-period ( P ≲ 10 days) binary systems in Transiting Exoplanet Survey Satellite data, 180 of which are heartbeat binaries. The sample is mostly a mix of A- and B-type stars and primarily includes eclipsing systems, where over 30% of ...
Siddhant Solanki +11 more
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Numerical Study on the Hydrodynamic Instability of Binary Stars in the First Post Newtonian Approximation of General Relativity [PDF]
M. Shibata, K. Oohara, Takashi Nakamura
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On the formation of single and binary helium-rich subdwarf O stars [PDF]
Stephen Justham +2 more
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Joint analysis of position measurements and radial velocities of six triple stellar systems is conducted to determine their inner and/or outer orbits. Accumulation of such data is needed to study the architecture of stellar hierarchies and its relation ...
Andrei Tokovinin
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