activity
20062024
most citedProperties and occurrence rates of exoplanet candidates as a function of host star metallicity from the DR25 catalog

71 citations · 679 across the 61 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2024

The Interaction Jigsaw: Investigating star formation in interacting galaxies

Thomas Robin, Sreeja S Kartha, Akhil Krishna R +5

Interaction between galaxies play a pivotal role in their evolution. Ongoing star formation in spiral galaxies can be affected by these processes. We select a sample of interacting…

astro-ph.SR2024

Study of the Balmer decrements for Galactic classical Be stars using the Himalayan Chandra Telescope of India

Gourav Banerjee, Blesson Mathew, Suman Bhattacharyya +3

In a recent study, Banerjee et al. (2021) produced an atlas of all major emission lines found in a large sample of 115 Galactic field Be stars using the 2-m Himalayan Chandra Teles…

astro-ph.GA2024

Beyond the Rings: Polar Ring Galaxy NGC 4262 and its Globular Cluster System

Akhil Krishna R, Sreeja S Kartha, Blesson Mathew

In the context of the hierarchical model of galaxy evolution, polar ring galaxies (PRGs) are considered the intermediate phase between ongoing mergers and quiescent galaxies. This…

astro-ph.SR2024

Chandra X-ray Analysis of Herbig Ae/Be Stars

Hema Anilkumar, Blesson Mathew, V. Jithesh +4

Herbig Ae/Be (HAeBe) stars are intermediate-mass pre-main sequence stars, characterized by infrared excess and emission lines. They are observed to emit X-rays, whose origin is a m…

astro-ph.GA2024

Gas kinematics and dynamics of Carina Pillars: A case study of G287.76-0.87

Ngo-Duy Tung, Le Ngoc Tram, Archana Soam +4

We study the kinematics of a pillar, namely G287.76-0.87, using three rotational lines of CO(5-4), CO(8-7), CO(11-10), and a fine structure line of [OI] $63\,μ…

astro-ph.SR2024

Optical Spectroscopy of Classical Be Stars in Old Open Clusters

Madhu Kashyap Jagadeesh, Blesson Mathew, K. T. Paul +4

We performed the optical spectroscopy of 16 classical Be stars in 11 open clusters older than 100 Myr. Ours is the first spectroscopic study of classical Be stars in open clusters…