activity
20032023
most citedMassive Quiescent Cores in Orion. I. Temperature Structure

56 citations · 129 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023★ 14 cited

A panoptic view of the Taurus molecular cloud I. The cloud dynamics revealed by gas emission and 3D dust

J. D. Soler, C. Zucker, J. E. G. Peek +14

We present a study of the three-dimensional (3D) distribution of interstellar dust derived from stellar extinction observations toward the Taurus molecular cloud (MC) and its relat…

astro-ph.GA2023★ 7 cited

CO enhancement by magnetohydrodynamic waves; Striations in the Polaris Flare

R. Skalidis, K. Gkimisi, K. Tassis +4

The formation of molecular gas in interstellar clouds is a slow process, but is enhanced by gas compression. Magnetohydrodynamic (MHD) waves create compressed quasiperiodic linear…

astro-ph.GA2023★ 18 cited

The Co-Ordinated Radio and Infrared Survey for High-Mass Star Formation. V. The CORNISH-South Survey and Catalogue

T. Irabor, M. G. Hoare, M. Burton +32

We present the first high spatial resolution radio continuum survey of the southern Galactic plane. The CORNISH project has mapped the region defined by $295^{\circ} < l < 350^{\ci…

astro-ph.GA2023★ 18 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -XIII. Ongoing triggered star formation within clump-fed scenario found in the massive ( ) clump

S. Zhang, K. Wang, T. Liu +16

Whether ionization feedback triggers the formation of massive stars is highly debated. Using ALMA 3 mm observations with a spatial resolution of pc and a mass sensitivi…

astro-ph.GA2021★ 16 cited

The "Maggie" filament: Physical properties of a giant atomic cloud

J. Syed, J. D. Soler, H. Beuther +19

The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associat…

astro-ph2003★ 56 cited

Massive Quiescent Cores in Orion. I. Temperature Structure

D. Li, P. F. Goldsmith, K. Menten

We have mapped four massive cores in Orion using the \ammonia (J,K) = (1,1) and (J,K) = (2,2) inversion transitions, as part of our effort to study the pre--protostellar phase of m…