activity
20212024
most citedGaia 20eae: A newly discovered episodically accreting young star

18 citations · 30 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2024

The Dusty Aftermath of a Rapid Nova: V5579 Sgr

A. Raj, M. S. Bisht, F. M. Walter +10

V5579 Sgr was a fast nova discovered in 2008 April 18.784 UT. We present the optical spectroscopic observations of the nova observed from the Castanet Tolosan, SMARTS and CTIO obse…

astro-ph.SR2024

Initial results of our spectro-photometric monitoring of XZ Tau

Arpan Ghosh, Saurabh Sharma, Joe Philip Ninan +5

We present here initial results of our spectro-photometric monitoring of XZ Tau. During our monitoring period, XZ Tau exhibited several episodes of brightness variations in timesca…

astro-ph.GA2024

Deciphering the Hidden Structures of HH 216 and Pillar IV in M16: Results from JWST and HST

L. K. Dewangan, O. R. Jadhav, A. K. Maity +6

To probe the star formation process, we present an observational investigation of the Pillar IV and an ionized knot HH 216 in the Eagle Nebula (M16). Pillar IV is known to host a C…

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.SR2023

Post-outburst evolution of bonafide FUor V2493 Cyg: A Spectro-photometric monitoring

Arpan Ghosh, Saurabh Sharma, Joe P. Ninan +11

We present here the results of eight years of our near-simultaneous optical/near-infrared spectro-photometric monitoring of bonafide FUor candidate `V2493 Cyg' starting from 2013 S…

astro-ph.SR20235 cited

Spectroscopy of 9 eruptive young variables using TANSPEC

Arpan Ghosh, Saurabh Sharma, Joe P. Ninan +8

In recent times, 3.6m Devasthal Optical Telescope (DOT) has installed an optical to near infra-red spectrograph, TANSPEC, which provides spectral coverage from 0.55-2.5 microns. Us…