activity
20062023
most citedThe rise of SN2014J in the nearby galaxy M82

132 citations · 584 across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2023

Polarimetric Approach Towards Membership Probability of Open Star Cluster NGC 2345

Sadhana Singh, Jeewan C. Pandey, Vishal Joshi

Using the linear polarimetric observations, we present a method to derive the membership probability of stars in cluster NGC 2345. The polarimetric observations of cluster NGC 2345…

astro-ph.SR2023

Snowflakes in a furnace: formation of CO and dust in a recurrent nova eruption

D. P. K. Banerjee, C. E. Woodward, V. Joshi +7

We report the detection of carbon monoxide (CO) and dust, formed under hostile conditions, in recurrent nova V745 Sco about 8.7 days after its 2014 outburst. The formation of molec…

astro-ph.SR2021★ 11 cited

Optical and near-infrared spectroscopy of Nova V2891 Cygni: evidence for shock-induced dust formation

Vipin Kumar, Mudit K. Srivastava, Dipankar P. K. Banerjee +6

We present multi-epoch optical and near-infrared observations of the highly reddened, \pion{Fe}{ii} class slow nova V2891 Cygni. The observations span 15 months since its discovery…

astro-ph.SR2021★ 4 cited

V838 Monocerotis as seen by ALMA: a remnant of a binary merger in a triple system

Tomek Kamiński, Romuald Tylenda, Aleksandra Kiljan +6

V838 Mon erupted in 2002 quickly becoming the prototype of a new type of stellar eruptions known today as (luminous) red novae. The red nova outbursts are thought to be caused by s…

astro-ph.SR2021★ 4 cited

Interplanetary magnetic flux rope observed at ground level by HAWC

S. Akiyama, R. Alfaro, C. Alvarez +59

We report the ground-level detection of a Galactic Cosmic-Ray (GCR) flux enhancement lasting 17 hr and associated with the passage of a magnetic flux rope (MFR) over the Ear…

astro-ph.HE2020★ 9 cited

Multi-wavelength view of the galactic black-hole binary GRS 1716-249

Sandeep K. Rout, Santosh V. Vadawale, Aarthy E. +5

The origins of X-ray and radio emissions during an X-ray binary outburst are comparatively better understood than those of ultraviolet, optical and infrared radiation. This is beca…