Results 61 to 70 of about 186,944 (198)
Detailed Analysis of Six Contact Binaries and their Possible Origin
A photometric investigation of six binary systems of the W Ursae Majoris (W UMa)-type is presented. We extracted primary and secondary minima from the Transiting Exoplanet Survey Satellite observations of these systems.
Somayeh Soomandar +2 more
doaj +1 more source
Roche Configurations of Two Near-Contact Binaries do CAS and SW Lyn [PDF]
Light curves of two near-contact binaries DO Cas and SW Lyn are analyzed to investigate their Roche configurations. We made new BVR observations for DO Cas and employed the published observation data for SW Lyn.
Ho-Il Kim +4 more
doaj
The New Contact Binary GSC 2414-0797 [PDF]
GSC 2414-0797 has a contact binary star type light curve, a 0.4 magnitude brightness variation with a period 0.3406 ...
Greimel, R. +5 more
core
Longitudinal associations between CBO contact and binary outcomes.
Longitudinal associations between CBO contact and binary outcomes.
Imca S. Hensels (3181011) +6 more
core +1 more source
Modelling the Delay Distribution of Binary Spray and Wait Routing Protocol [PDF]
His article proposes a stochastic model to obtain the end-to-end delay law between two nodes of a Delay Tolerant Network (DTN). We focus on the commonly used Binary Spray and Wait (BSW) routing protocol and propose a model that can be applied to ...
Emmanuel Lochin +3 more
core +1 more source
Detection of Contact Binary Candidates Observed By TESS Using the Autoencoder Neural Network
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 +1 more source
Near-Contact Binaries on the Path to Contact Binaries
22 pages, 5 figures, to appear in Acta ...
openaire +2 more sources
Fundamental Parameters for Totally Eclipsing Contact Binaries Observed by TESS
Totally eclipsing contact binaries provide a unique opportunity to accurately determine mass ratios through photometric methods alone, eliminating the need for spectroscopic data.
Xu Ding +7 more
doaj +1 more source
A Analysis of the Light and Radial Velocity Curves of do CAS [PDF]
DO Cas is a short period (P=0.68day) eclipsing binary star and is classified as a near-contact binary by Shaw (1990). There is no published radial velocity curve for this short period binary after Mannino (1958).
Young Sook Ahn, Ho-Il Kim, Woo-Baik Lee
doaj
Photometric Study of a W UMa Type Contact Binary AH CNC [PDF]
CCD photometric observations of a W UMa type contact binary AH Cnc were performed for ten nights from December 1998 to May 1999 using a PM512 CCD camera and BVI filters attached to the 61cm reflector at Sobaeksan Optical Astronomy Observatory.
Jae-Hyuck Youn +6 more
doaj +1 more source

