activity
20082025
most citedAn Approach to Estimate the Binding energy of Interstellar Species

74 citations · 1k across the 41 of their papers we have counts for

collaborators

41 papers

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.SR2023

Chemical evolution of some selected complex organic molecules in low-mass star-forming regions

Bratati Bhat, Rumela Kar, Suman Kumar Mondal +6

The destiny of complex organic molecules (COMs) in star-forming regions is interlinked with various evolutionary phases. Therefore, identifying these species in diversified environ…

astro-ph.GA2023★ 33 cited

Digging into the Interior of Hot Cores with ALMA (DIHCA). III: The Chemical Link between NHCHO, HNCO, and HCO

Kotomi Taniguchi, Patricio Sanhueza, Fernando A. Olguin +8

We have analyzed the NHCHO, HNCO, HCO, and CHCN (CHCN) molecular lines at an angular resolution of obtained by the Atacama Large Millime…

astro-ph.GA2022★ 14 cited

Investigating the hot molecular core, G10.47+0.03: A pit of nitrogen-bearing complex organic molecules

Suman Kumar Mondal, Wasim Iqbal, Prasanta Gorai +3

Recent observations have shown that Nitrogen-bearing complex organic species are present in large quantities in star-forming regions. Thus, investigating the N-bearing species in a…

astro-ph.GA2022★ 14 cited

Astrochemical model to study the abundances of branched carbon-chain molecules in a hot molecular core with realistic binding energies

Satyam Srivastav, Milan Sil, Prasanta Gorai +3

Straight-chain (normal-propyl cyanide, n - C3H7CN) and branched-chain (iso-propyl cyanide, i - C3H7CN) alkyl cyanides are recently identified in the massive star-forming regions (S…

astro-ph.GA2021★ 10 cited

Radiative transfer modeling of the observed line profiles in G31.41+0.31

Bratati Bhat, Prasanta Gorai, Suman Kumar Mondal +2

An inverse P-Cygni profile of H13CO+ (1-0) in G31.41+0.31 was recently observed, which indicates the presence of an infalling gas envelope. Also, an outflow tracer, SiO, was observ…