109 citations · 1.1k across the 59 of their papers we have counts for
7 papers · 1 filter
The magnetic field in the dense photodissociation region of DR 21
Atanu Koley, Nirupam Roy, Karl M. Menten +3
Measuring interstellar magnetic fields is extremely important for understanding their role in different evolutionary stages of interstellar clouds and of star formation. However, d…
A population of hypercompact HII regions identified from young HII regions
Aiyuan Yang, James Urquhart, Mark Thompson +8
Context. The derived physical parameters for young HII regions are normally determined assuming the emission region to be optically thin. However, this assumption is unlikely to ho…
Large-scale Map of Millimeter-wavelength Hydrogen Radio Recombination Lines around a Young Massive Star Cluster
Q. Nguyen-Luong, L. D. Anderson, L. D. +19
We report the first map of large-scale (10 pc in length) emission of millimeter-wavelength hydrogen recombination lines (mm-RRLs) toward the giant H II region around the W43-Main y…
Atomic and molecular gas properties during cloud formation
J. Syed, Y. Wang, H. Beuther +15
Molecular clouds, which harbor the birthplaces of stars, form out of the atomic phase of the interstellar medium (ISM). We aim to characterize the atomic and molecular phases of th…
Synthetic observations of spiral arm tracers of a simulated Milky Way analog
Stefan Reissl, Jeroen M. Stil, En Chen +16
Context: The Faraday rotation measure (RM) is often used to study the magnetic field strength and orientation within the ionized medium of the Milky Way. Observations indicate a RM…
The history of dynamics and stellar feedback revealed by the HI filamentary structure in the disk of the Milky Way
J. D. Soler, H. Beuther, J. Syed +19
We present a study of the filamentary structure in the emission from the neutral atomic hydrogen (HI) at 21 cm across velocity channels in the 40'' and 1.5-km/s resolution position…
Cloud formation in the atomic and molecular phase: HI self absorption (HISA) towards a Giant Molecular Filament
Y. Wang, S. Bihr, H. Beuther +20
Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular interstellar medium (ISM) is a d…