activity
20172026
most citedThe disintegrating old open cluster Czernik 3

32 citations · 193 across the 26 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2026

Bridging the gap between stars and planets

Aina Palau, Dimitris Stamatellos, Matthew Bate +58

The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these…

astro-ph.SR2026

Unveiling the First O-Type Bloated Star Candidate through ALMA and EVLA Observations

Rakesh Pandey, Aina Palau, Alvaro Sánchez-Monge +5

We investigate the circumstellar environment of the O-type bloated star candidate IRAS 19520+2759 (I19520) using high-resolution observations from the Atacama Large Millimeter/subm…

astro-ph.SR2025

Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability

Rakesh Pandey, Aina Palau, Javier Serna +8

Using optical time series with Telescopi Joan Oró (TJO), Gaia, TESS, and NEOWISE archival data, we performed a variability study on the candidate bloated massive young stellar obje…

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.SR2023★ 1 cited

Identifying the population of T-Tauri stars in Taurus: UV-optical synergy

Prasanta K. Nayak, Mayank Narang, Manoj Puravankara +9

With the third data release of the Gaia mission DR3 with its precise photometry and astrometry, it is now possible to study the behaviour of stars at a scale never seen befo…