Activity of the first interstellar comet 2I/Borisov around perihelion: Results from Indian observatories
Aravind Krishnakumar (1, 2), Shashikiran Ganesh (1), Kumar, Venkataramani (3), Devendra Sahu (4), Dorje Angchuk (4), Thirupathi Sivarani, (4), Athira Unni (4) ((1) Physical Research Laboratory, Ahmedabad, India,(2), Institute of Technology Gandhinagar, Gandhinagar, India

TL;DR
This study presents observational results of interstellar comet 2I/Borisov from Indian observatories, revealing its molecular composition, surface heterogeneity, and dust-to-gas ratio, showing similarities to Solar system comets.
Contribution
First detailed observational analysis of 2I/Borisov from Indian observatories, highlighting its molecular composition, surface heterogeneity, and physical properties.
Findings
CN was the dominant molecular emission at both epochs.
The comet is moderately depleted in carbon chain molecules.
Its behavior is similar to Solar system comets.
Abstract
Comet 2I/Borisov is the first true interstellar comet discovered. Here we present results from observational programs at two Indian observatories, 2 m Himalayan Chandra Telescope at the Indian Astronomical Observatory, Hanle (HCT) and 1.2 m telescope at the Mount Abu Infrared Observatory (MIRO). Two epochs of imaging and spectroscopy were carried out at the HCT and three epochs of imaging at MIRO. We found CN to be the dominant molecular emission on both epochs, 31/11/2019 and 22/12/2019, at distances of r = 2.013 and 2.031 AU respectively. The comet was inferred to be relatively depleted in Carbon bearing molecules on the basis of low and abundances. We find the production rate ratio, Q()/Q(CN) = 0.54 0.18, pre-perihelion and Q()/Q(CN) = 0.34 0.12 post-perihelion. This classifies the comet as being moderately depleted in carbon chain molecules.…
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