12 citations · 16 across the 7 of their papers we have counts for
7 papers
The Close Binary V486 Carinae
Ahmet Erdem, Volkan Bakis, Burcu Ozkardes +5
The hitherto neglected close binary V486 Car is studied with the aid of newly applied satellite photometry (HIPPARCOS and TESS), high dispersion spectrometry (HERCULES) and ground-…
BSN-VI: Multiband Light Curve Modeling of Four W UMa-Type Contact Binaries I. Revisiting Energy Transfer Mechanisms and Luminosity Behavior
Elham Sarvari, Atila Poro, Raul Michel +5
We presented the first high-precision, detailed photometric analysis of four W Ursae Majoris (W UMa)-type contact binaries, Linear 10772300, Linear 11150338, Linear 20372537 and DM…
Quadruple system HD 135160 in a unique 2+2 configuration
Michal Zummer, Petr Harmanec, Brad Barlow +2
Analysing a large body of observational data, we found that HD 135160 is a quadruple 2+2 system, composed of a massive ellipsoidal binary ('heartbeat' star) with components Aa and…
Absolute Parameters of Young Stars: NO Puppis
Ahmet Erdem, Volkan Bakış, John Southworth +6
The southern early-type, young, eccentric-orbit eclipsing binary NO Puppis forms the A component of the multiple star Gaia DR3 552\-8147999779517568. The B component is an astromet…
Comparative study of the W UMa type binaries S Ant and Epsilon CrA
Volkan Bakis, Edwin Budding, Ahmet Erdem +6
Contact binaries challenge contemporary stellar astrophysics with respect to their incidence, structure and evolution. We explore these issues through a detailed study of two brigh…
The First Photometric Study of AH Mic Contact Binary System
Atila Poro, Mark G. Blackford, Selda Ranjbar Salehian +7
The first multi-color light curve analysis of the AH Mic binary system is presented. This system has very few past observations from the southern hemisphere. We extracted the minim…
Absolute Parameters of Young Stars: V Puppis
Edwin Budding, Tom Love, Mark G. Blackford +2
New spectrometric data on V Pup are combined with satellite photometry (HIPPARCOS and recent TESS) to allow a revision of the absolute parameters with increased precision. We find:…