activity
20082026
most citedVLTI monitoring of the dust formation event of the Nova V1280 Sco

40 citations · 76 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Optical Spectroscopy and Temporal Evolution of the Nova V1405 Cas

Gesesew R. Habtie, Ramkrishna Das, Elias Aydi +1

This paper presents the findings from our study of nova V1405~Cas over the first 1051 days after the outburst. The study includes an analysis of the photometric light curve evoluti…

astro-ph.GA2024★ 5 cited

Fate and detectability of rare gas hydride ions in nova ejecta: A case study with nova templates

Milan Sil, Ankan Das, Ramkrishna Das +6

HeH was the first heteronuclear molecule to form in the metal-free Universe after the Big Bang. The molecule gained significant attention following its first circumstellar dete…

astro-ph.SR2024

Spectroscopic study of the Quiescent Stages in between the 2006 and 2021 outbursts of RS Ophiuchi

Gesesew R. Habtie, Ramkrishna Das

This paper presents a comprehensive spectroscopic analysis of the quiescent stage of the recurrent nova RS Ophiuchi between its 2006 and 2021 outbursts. The spectra shows prominent…

astro-ph.SR2023★ 17 cited

Study of the fastest classical nova, V1674 Her: Photoionization and Morpho-kinemetic model analysis

Gesesew R. Habtie, Ramkrishna Das, Ruchi Pandey +2

We present the results of the investigation of the nova V1674 Her (2021), recognised as the swiftest classical nova, with days. The distance to the nova is estimate…

astro-ph.SR2013

Near-infrared spectroscopic and photometric evolution of Nova V476 Scuti -- a nova that formed optically thin dust

R. K. Das, D. P. K. Banerjee, N. M. Ashok +1

We present results of near-infrared (near-IR) (1.07 - 2.5 m) spectroscopic and photometric observations of Nova V476 Scuti (V476 Sct) which was discovered in outburst in 2…

astro-ph.SR2010★ 11 cited

Near-infrared studies of the 2010 outburst of the recurrent nova U Scorpii

D. P. K. Banerjee, R. K. Das, N. M. Ashok +6

We present near-IR observations of the 2010 outburst of U Sco. JHK photometry is presented on ten consecutive days starting from 0.59 days after outburst. Such photometry can gainf…