LOW MASS RATIO CONTACT BINARY V410 Aur AND V776 Cas-II [PDF]
New BVR CCD light curves of the low mass ratio contact binaries, V410 Aur and V776 Cas, were observed with the 61 cm reflector and a 2K CCD camera at the Sobaeksan Astronomical Observatory.
Chun-Hwey Kim, Ho-Il Kim
exaly +2 more sources
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
exaly +2 more sources
STATISTICAL SURVEY FOR THE PHYSICAL CHARACTERISTIC OF NEAR CONTACT BINARY(NCBs) [PDF]
The absolute dimensions and orbital elements of 66 near contact binaries, collected from literatures, have been analyzed to investigate the physical characteristics of the near contact binaries as well as co-relations among physical parameters.
Kyu-Dong Oh
exaly +2 more sources
Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network [PDF]
A contact binary may be the progenitor of a red nova that eventually produces a merger event and have a cut-off period of around 0.2 days. Therefore, a large number of contact binaries is needed to search for the progenitor of red novae and to study the ...
Xu Ding +3 more
doaj +2 more sources
CCD Photometry of Low Mass Ratio Contact Binary FP Boo - IV [PDF]
We present new B, V, and R CCD photometric light curves for the low mass ratio contact binary FP Boo. A new photometric solution and absolute physical dimensions of the system were derived by applying the Wilson-Devinney program to our observed light ...
Kyu-Dong Oh, Woo-Baik Lee
exaly +2 more sources
LOW MASS RATIO CONTACT BINARY SYSTEMS HN UMa AND II UMa - III [PDF]
We present newly observed BVRI CCD light curves for low mass ratio contact binaries, HN UMa and II UMa. The absolute dimensions of these objects were obtained by applying the Wilson-Devinney program to previously published spectroscopic analysis and to ...
Ho-Il Kim
exaly +2 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 +2 more sources
A Method of Rapidly Deriving Late-type Contact Binary Parameters and Its Application in the Catalina Sky Survey [PDF]
With the continuous development of large optical surveys, a large number of light curves of late-type contact binary systems (CBs) have been released.
JinLiang Wang +5 more
doaj +2 more sources
Effects of Metallicity on the Instability Mass Ratio of Low Mass Contact Binary Systems. [PDF]
The orbital stability of contact binary systems has been receiving considerable attention recently. Theoretical studies indicate that merger is likely to occur at very low mass ratios, but the actual mass ratio at which merger may take place is likely ...
S. Wadhwa +9 more
semanticscholar +1 more source
The first photometric and orbital period investigation of an extremely low mass ratio contact binary with a sudden period change, TYC 4002-2628-1 [PDF]
Photometric observations for the totally eclipsing binary system TYC 4002-2628-1, were obtained between November 2020 and November 2021. To determine the stellar atmospheric parameters, a spectral image was taken with the 2.16 m telescope at National ...
D. Guo +8 more
semanticscholar +1 more source

