Results 11 to 20 of about 2,626,294 (294)
Small Mass Ratio Contact Binary [PDF]
The contact binary system has been classified in five different types according to their physical properties.
Kyu-Dong Oh +3 more
doaj +6 more sources
The Strength and Shapes of Contact Binary Objects [PDF]
While contact binary objects are common in the solar system, their formation mechanism is unclear. In this work we examine several contact binaries and calculate the necessary strength parameters that allow the two lobes to merge without the smaller of ...
Alex J. Meyer, Daniel J. Scheeres
doaj +4 more sources
Small Mass Ratio Contact Binary GR Vir and HV Aqr [PDF]
The absolute dimensions of low mass contact binary, GR Vir and HV Aqr were obtained using WD program from the published spectroscopic and photometric observational data.
Kyu-Dong Oh +4 more
doaj +2 more sources
A Photometric Study of Near-Contact Binary ZZ Aur [PDF]
The BVR CCD full light curves of ZZ Aur were obtained as one of the near-contact binary observing programs at the Sobaek Mt. Observatory during Feb. 2000 - Feb. 2001. From the present observations, three primary and seven secondary times of minimum light
Kyu-Dong Oh +3 more
doaj +2 more sources
TV UMi: A Shallowly Eclipsing Marginal-Contact Binary
Using twenty sectors of TESS observations and the hitherto unutilized radial velocities from the David Dunlap Observatory survey, we fully characterize the close binary TV UMi.
Atila Čeki, Olivera Latković
doaj +2 more sources
Composite contact of binary lipid membranes
Upon adhesion, binary lipid membranes may retain their structural identity but they may also undergo partial fusion promoted by microscopic phase separation of the components. In membranes composed of cylindrical and inverted conical lipids, a partially fused contact zone may consist of inverted micelles sandwiched between two monolayers.
U, Jelerčič, P, Ziherl
openaire +3 more sources
Photoelectric Observations and Analysis of the Contact Binary W UMa [PDF]
The unpublished photoelectric observations of the contact binary W UMa in ultraviolet, blue, and yellow bandpasses made on four nights during the observing seasons from April, 1984 to May, 1985 were presented.
Chun-Hwey Kim +2 more
doaj +1 more source
Mass-ratio distribution of contact binary stars [PDF]
When the mass ratio of a contact binary system drops below the critical value $q_\mathrm{min}$, the binary undergoes the tidal Darwin instability, leading to a rapid merger and observable brightening.
Pešta, Milan
core +2 more sources
Context. Among massive stars, binary interaction is the rule rather than the exception. The closest binaries – those with periods of less than ∼10 days – undergo mass transfer during core-hydrogen burning, with many of them experiencing a nuclear-timescale contact phase.
Fabry, M. +3 more
+13 more sources
CN Trianguli: A W-type Contact Binary Exhibiting A-type Light Curve via Starspot-induced Dimming
We present comprehensive photometric observations and analysis of the totally eclipsing binary CN Tri. The photometric solutions suggest it as an extremely low mass ratio contact binary system with q ∼ 0.08.
Zhi-Hua Wang +3 more
doaj +2 more sources

