1 citations · 1 across the 6 of their papers we have counts for
7 papers
Investigating Variability in Long-lived Protoplanetary Disks (>10 Myr) using NEOWISE
Gregory Mathews Ben, Jessy Jose, Jesús Hernández
We present the mid-infrared variability study of 120 long-lived disk candidates (ages 10-100 Myr) and 13 confirmed "Peter Pan" disks using NEOWISE to constrain the longevity of dyn…
Magnetic field Topology and Star Formation in the Cepheus B Filamentary cloud under External Feedback
Panigrahy Sandhyarani, Chakali Eswaraiah, Manash R. Samal +6
We present a detailed study of the Cep B molecular cloud based on sub-mm dust polarization and CO (J=3--2) spectral line observations obtained with SCUBA-2/POL-2 and HARP on…
Investigating the Influence of Radiative Feedback in Bright-Rimmed Cloud 44
Rishi C, Neelam Panwar, Thomas J. Haworth +9
Radiative feedback from massive stars plays a central role in the evolution of molecular clouds and the interstellar medium. This paper presents a multi-wavelength analysis of the…
Protoplanetary Disk Survival Time-scales: A Blind Survey of Young Clusters up to 100 Myr in the Solar Vicinity
Gregory Mathews Ben, Jessy Jose, Jesús Hernández
We study the protoplanetary disk lifetimes using a large sample of young stellar objects in nearby clusters. To investigate the final phase of disk dissipation, we selected 32 clus…
Variation of Dense Gas Mass-Luminosity conversion factor with metallicity in the Milky Way
Sudeshna Patra, Neal J. Evans, Kee-Tae Kim +10
HCN and HCO are the most common dense gas tracers used both in the Milky Way and external galaxies. The luminosity of HCN and HCO lines are converted to a dense g…
Does Metallicity affect Protoplanetary Disk Fraction? Answers from the Outer Milky Way
Sudeshna Patra, Jessy Jose, Neal J. Evans
The role of metallicity in shaping protoplanetary disk evolution remains poorly comprehended. This study analyzes the disk fraction of 10 young (0.9-2.1 Myr) and low-metallicity (0…
The role of magnetic fields in the fragmentation of the Taurus B213 filament into Sun-type star-forming cores
Anirudh R., Chakali Eswaraiah, Sihan Jiao +1
Fragmentation is a key step in the process of transforming clouds (and their substructures such as filaments, clumps, and cores) into protostars. The thermal gas pressure and gravi…