activity
20172025
most citedThe ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

37 citations · 168 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

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

Low-mass stellar and substellar content of the young cluster Berkeley 59

Neelam Panwar, Rishi C., Saurabh Sharma +4

We present a multi-wavelength analysis of the young star cluster Berkeley 59 (Be 59) based on the data and deep infrared (IR) observations with the 3.58-m Telescopio Naziona…

astro-ph.GA2023

Cluster Formation in a Filamentary Cloud: The Case of the Stellar Cluster NGC 2316

Saurabh Sharma, Aayushi Verma, Kshitiz Mallick +7

We present a multi-wavelength analysis of the star cluster NGC 2316 and its surroundings. We estimated the physical parameters of the NGC 2316 cluster, including its shape (elongat…

astro-ph.GA2023

Dissecting the morphology of star forming complex S193

Rakesh Pandey, Saurabh Sharma, Lokesh Dewangan +5

We have studied a star-forming complex S193 using near-infrared (NIR) observations and other archival data covering optical to radio wavelengths. We identified stellar clusters in…

astro-ph.GA2023

Exploring Stellar Cluster and Feedback-driven Star Formation in Galactic Mid-infrared Bubble [HKS2019] E70

Aayushi Verma, Saurabh Sharma, Kshitiz K. Mallick +8

We present a comprehensive analysis of the Galactic mid-infrared (MIR) bubble [HKS2019] E70 (E70) by adopting a multi-wavelength approach to understand the physical environment and…

astro-ph.GA20226 cited

Diagnosing Triggered Star Formation in the Galactic H II region Sh 2-142

Tanvi Sharma, Wen Ping Chen, Neelam Panwar +2

Stars are formed by gravitational collapse, spontaneously or, in some cases under the constructive influence of nearby massive stars, out of molecular cloud cores. Here we present…