39 citations · 145 across the 47 of their papers we have counts for
48 papers
Statistical structure and physical interpretation of the fillout factor distribution in contact binary stars
A. Poro, K. Li, E. Paki +2
Contact binary systems exhibit complex evolutionary behavior governed by mass transfer, angular momentum loss (AML), and Roche geometry. The fillout factor () is widely used as…
BSN-VII: Photometric Light Curve Study of Three Cool, Large-Amplitude, Low Mass, W-Subtype Contact Binaries
Atila Poro, Raul Michel, Diana Zadkhosh +9
We present a comprehensive photometric study of three W UMa-type contact binary systems, V1104 Her, V1284 Her, and V2822 Ori, based on a combination of ground-based observations an…
BSN-VIII: Detailed Photometric Modeling of Ten W UMa Contact Binaries and a Revised Empirical Period-Mass Relationship
Atila Poro, S. Javad Jafarzadeh, Kai Li +15
This study continues our ongoing research on contact binary systems by presenting a detailed analysis of 10 targets. Ground-based observations from six different observatories were…
BSN: Light Curve Modeling and Orbital Period Analysis of the Contact Binaries OV Leo and V339 Leo
Razieh Aliakbari, Atila Poro, Raul Michel +1
We present a combined photometric and orbital period analysis of the contact binary systems OV Leo and V339 Leo using ground-based observations together with TESS photometry. The l…
Multivariate Statistical Analysis of Low Mass Ratio Contact Binaries: Definition, Dynamical Stability, and Parameter Relationships
A. Poro, R. Poggiani, A. Foroutanfar +3
This study explores multiple aspects of W Ursae Majoris (W UMa) contact binary systems with low mass ratios, providing empirical insights into their definition, structure, rotation…
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…
Detailed TESS-Based Light Curve Modeling and Fundamental Parameter Estimation of 27 W UMa-Type Contact Binaries
Atila Poro, Ahmad Sarostad, Mohammad Davoudi +30
We performed a comprehensive analysis of 27 short period contact binary systems for which no light curve analysis had previously been reported. Photometric time-series data from th…
Detailed Investigation of a W UMa Contact Binary with an Ultralow Mass Ratio and a Third-Body as a Potential Merger Candidate
Atila Poro, Ehsan Paki, Fahri Alicavus +1
The lower limit of the mass ratio in contact binaries remains uncertain, with observations suggesting systems exist below theoretical predictions. The stability of such very low ma…
BSN: Light Curve Modeling and Orbital Evolution of the Total-Eclipse Contact Binary EZ Oct
Asma Ababafi, Atila Poro, Mehmet Tanriver +1
We present the first detailed multiband (BVR_cI_c and TESS) photometric analysis of the short-period binary EZ Oct. This study combines ground-based observations conducted at a Sou…
BSN: The First Multiband Light Curve Analysis of the W UMa-type Contact Binary System EM Tucanae
Sepideh Houshiar, Atila Poro, Abbas Abedini +1
We present a comprehensive photometric light curve and orbital period analysis of the W UMa-type contact binary EM Tuc. The O-C analysis constructed from all available eclipse timi…
BSN-V: The First Detailed Light Curve Modeling of Eight Totally Eclipsing Contact Binary Stars Using Ground-Based and TESS Observations
Atila Poro, Raul Michel, Francisco Javier Tamayo +3
This study broadens our comprehensive investigation of total-eclipse W Ursae Majoris-type contact binaries by analyzing eight additional systems, continuing our previous research.…
BSN-IV: The First Multiband Light Curve Study of Five W UMa-type Contact Binary Systems
Atila Poro, Raul Michel, Jean-François Coliac +6
In this work, we present a detailed investigation of five contact binary systems of the W Ursae Majoris (W UMa) type. Multiband photometric observations were conducted using ground…
Asteroid Rotation Periods: Statistical Analysis in the Diameter-Spin Distribution
Maryam Nastaran, Atila Poro, Raziyeh Hosseini +1
This study examines the rotational characteristics of asteroids through statistical modeling of the diameter-period relationship. A statistical evaluation of the diameter-period re…
BSN-II: The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors
Atila Poro, Kai Li, Raul Michel +6
This study provides the first comprehensive analysis of eight total-eclipse W Ursae Majoris-type contact binary systems. Ground-based photometric multiband observations were conduc…
The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems
Ehsan Paki, Atila Poro, Minoo Dokht Moosavi Rowzati
Light curve analysis of W UMa-type contact binary systems using MCMC or MC methods can be time-consuming, primarily because the repeated generation of synthetic light curves tends…
BSN-III: The First Multiband Photometric Study on the Eight Total Eclipse Contact Binary Stars
Atila Poro, Kai Li, Raul Michel +6
This study continues our in-depth investigation of total-eclipse W Ursae Majoris-type contact binaries by analyzing eight new systems, complementing our previous work. Multiband $B…
Four Total Eclipsing Contact Binary Systems: The First Photometric Light Curve Solutions Employing TESS and Gaia Surveys
Atila Poro, Razieh Aliakbari, Hossein Azarara +2
We presented the first photometric light curve solutions of four W Ursae Majoris (W UMa)-type contact binary systems. This investigation utilized photometric data from the Transiti…
The First In-depth Photometric Study of the Four Delta Scuti Stars Using TESS Data
Atila Poro, Hossein Azarara, Ahmad Sarostad +4
The first in-depth photometric study of four Delta Scuti stars was performed. We used time series data from the Transiting Exoplanet Survey Satellite (TESS) that is available in di…
BSN: The First Photometric Analysis of Contact Binary Systems V1961 Cyg and V0890 Lyr
Sabrina Baudart, Atila Poro
We presented the first photometric analysis of the V1961 Cyg and V0890 Lyr binary systems. We observed and analyzed these systems at an observatory in France as part of the Binary…
BSN: The First Light Curve Analysis of the Total Eclipse Binary System EL Tuc
Elham Sarvari, Eduardo Fernández Lajús, Atila Poro
We conducted the first light curve study of the binary star EL Tuc within the Binary Systems of South and North (BSN) Project framework. The photometric observations were made usin…
Reanalyzing the Light Curves and Absolute Parameters of Twenty Contact Binary Stars Using TESS Data
Ehsan Paki, Atila Poro
Reanalyzing contact binaries with space-based photometric data and investigating possible parameter changes can yield accurate samples for theoretical studies. We investigated ligh…
BSN: First Photometric Light Curve Analysis of Two W-type Contact Binary Systems OP Boo and V0511 Cam
Atila Poro, Mehmet Tanriver, Ahmet Keskin +5
This study presented the first light curve analysis of the OP Boo and V0511 Cam binary stars, which was conducted in the frame of the Binary Systems of South and North (BSN) Projec…
First Light Curve Analysis of NSVS 8294044, V1023 Her, and V1397 Her Contact Binary Systems
Atila Poro, Sabrina Baudart, Mahshid Nourmohammad +7
The first photometric light curve investigation of the NSVS 8294044, V1023 Her, and V1397 Her binary systems is presented. We used ground-based observations for the NSVS 8294044 sy…
Estimating the Absolute Parameters of W UMa-type Binary Stars Using Gaia DR3 Parallax
Atila Poro, Mahya Hedayatjoo, Maryam Nastaran +7
The accuracy of absolute parameters' estimation in contact binary systems is important for investigating their evolution and solving some challenges. The Gaia DR3 parallax is one o…