Gravitational interaction signatures in isolated galaxy triplet systems: a photometric analysis
Amira A. Tawfeek, Kanak Saha, Kaustubh Vaghmare, Ajit Kembhavi, Ali, Takey, Bernardo Cervantes Sodi, Jacopo Fritz, Zainad Awad, Gamal B. Ali,, Hayman Zain

TL;DR
This study analyzes nine isolated galaxy triplet systems using photometric methods, revealing that most member galaxies show signs of interaction, indicating these systems are physically bound and dynamically active.
Contribution
It provides the first detailed photometric analysis of isolated galaxy triplets, demonstrating prevalent interaction signatures through 1D and 2D surface brightness profile modeling.
Findings
55% of disk galaxies are type III, indicating interactions.
70% of galaxies show asymmetric features and signs of interaction.
Galaxy triplets with small projected separations are physically bound and interacting.
Abstract
Galaxy triplets are interesting laboratories where we can study the formation and the evolution of small and large systems of galaxies. This study aims to investigate signs of interaction between the members of nine isolated galaxy triplet systems (27 galaxies) selected from the "SDSS-based catalogue of Isolated Triplets" (SIT) with members brighter than 17.0 ( 17.0) in the band, and mean projected separation between the members of 0.1 Mpc. In this work, we performed a one-dimensional (1D) fitting of the surface brightness profiles and a two-dimensional (2D) modeling of the sample galaxies. In the 1D fitting, we examined the far outer part of the light profiles of disk galaxies (22 galaxies) and categorized them into type I (simple exponential), type II (down-bending), and type III (up-bending). This fitting results showed that 55 of disk galaxies in our…
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