activity
20242026
collaborators

6 papers

astro-ph.SR2026

Gaia24ccy: An outburst followed the footsteps of its predecessor

Koshvendra Singh, Joe P. Ninan, Zhen Guo +25

Accretion-driven outbursts in young stellar objects remain poorly understood, largely limited by a statistically small sample of closely followed-up events. This underscores the im…

astro-ph.SR2026

Unveiling the First O-Type Bloated Star Candidate through ALMA and EVLA Observations

Rakesh Pandey, Aina Palau, Alvaro Sánchez-Monge +5

We investigate the circumstellar environment of the O-type bloated star candidate IRAS 19520+2759 (I19520) using high-resolution observations from the Atacama Large Millimeter/subm…

astro-ph.SR2025

Investigating the Influence of Radiative Feedback in Bright-Rimmed Cloud 44

Rishi C, Neelam Panwar, Thomas J. Haworth +9

Radiative feedback from massive stars plays a central role in the evolution of molecular clouds and the interstellar medium. This paper presents a multi-wavelength analysis of the…

astro-ph.GA2025

Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective

Bhaswati Mookerjea, Maheswar G., Kinsuk Acharyya +24

Although the star formation process has been studied for decades, many important aspects of the physics involved remain unsolved. Recent advancement of instrumentation in the infra…

astro-ph.GA2024

Peering into the Heart of the Giant Molecular Cloud G148.24+00.41: A Deep Near-infrared View of the Newly Hatched Cluster FSR 655

Vineet Rawat, M. R. Samal, D. K. Ojha +5

We present a detailed near-infrared study of an embedded cluster located in the hub of the giant molecular cloud G148.24+00.41 of mass 10 , with the TANSPEC inst…

astro-ph.GA2024

Star formation exists in all early-type galaxies -- evidence from ubiquitous structure in UV images

Divya Pandey, Sugata Kaviraj, Kanak Saha +1

Recent surveys have demonstrated the widespread presence of UV emission in early-type galaxies (ETGs), suggesting the existence of star formation in many of these systems. However,…