activity
20012022
most citedUnifying low and high mass star formation through density amplified hubs of filaments

168 citations · 1.7k across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.SR2022★ 9 cited

A Study of the Magnetic Activity and Variability of GJ 436

M. Kumar, R. Fares

We present a magnetic activity study of GJ 436 using spectroscopic data from HARPS, spanning over 14 years, and additional data from NARVAL, falling within the HARPS observations.…

astro-ph.HE2022★ 29 cited

Faint light of old neutron stars and detectability at the James Webb Space Telescope

Shiuli Chatterjee, Raghuveer Garani, Rajeev Kumar Jain +3

Isolated ideal neutron stars (NS) of age yrs exhaust thermal and rotational energies and cool down to temperatures below K. Accretion of particle dark ma…

astro-ph.GA2022★ 18 cited

Cloud-cloud collision as origin of the G31.41+0.31 massive protocluster

M. T. Beltrán, V. M. Rivilla, M. S. N. Kumar +2

The G31.41+0.31 (G31) hot molecular core (HMC) is a high-mass protocluster showing accelerated infall and rotational spin-up that is well studied at high-angular resolution. To com…

astro-ph.GA2022★ 17 cited

The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31

M. T. Beltrán, V. M. Rivilla, R. Cesaroni +15

Context. To better understand the formation of high-mass stars, it is fundamental to investigate how matter accretes onto young massive stars, how it is ejected, and how all this d…

astro-ph.GA2022★ 48 cited

Filament coalescence and hub structure in MonR2: Implications to massive star and cluster formation

M. S. N. Kumar, D. Arzoumanian, A. Men'shchikov +3

Here we study the MonR2 star forming region, which has a rich network of filaments joining in a star cluster forming hub, aiming at understanding the hub structure and to examine t…

astro-ph.SR2021★ 33 cited

Analysis of physical processes in eruptive YSOs with near infrared spectra and multi-wavelength light curves

Zhen Guo, P. W. Lucas, C. Contreras Peña +11

The decade-long Vista Variables in the Via Lactea (VVV) survey has detected numerous highly variable young stellar objects (YSOs). We present a study of 61 highly variable VVV YSOs…