activity
20032022
most citedMolecular gas kinematics within the central 250 pc of the Milky Way

231 citations · 2k across the 51 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.GAShow all

5 papers · 2 filters

astro-ph.GA2018★ 21 cited

A Centimeter-wave Study of Methanol and Ammonia Isotopologues in Sgr B2(N): Physical and chemical differentiation between two hot cores

E. A. C. Mills, J. Corby, A. R. Clements +4

We present new radio-frequency interferometric maps of emission from the 14NH3, 15NH3, and 14NH2D isotopologues of ammonia, and the 12CH3OH and 13CH3OH isotopologues of methanol to…

astro-ph.GA2018★ 76 cited

Relative Alignment Between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud using Low and High Density Tracers

Laura M. Fissel, Peter A. R. Ade, Francesco E. Angilè +37

We compare the magnetic field orientation for the young giant molecular cloud Vela C inferred from 500-m polarization maps made with the BLASTPol balloon-borne polarimeter to th…

astro-ph.GA2018★ 2 cited

Low-Frequency Carbon Recombination Lines in the Orion Molecular Cloud Complex

Chenoa D. Tremblay, Christopher H. Jordan, Maria Cunningham +2

We detail tentative detections of low-frequency carbon radio recombination lines from within the Orion molecular cloud complex observed at 99-129 MHz. These tentative detections in…

astro-ph.GA2018★ 28 cited

The properties of Planck Galactic cold clumps in the L1495 dark cloud

Mengyao Tang, Tie Liu, Sheng-Li Qin +19

Planck Galactic Cold Clumps (PGCCs) possibly represent the early stages of star formation. To understand better the properties of PGCCs, we studied 16 PGCCs in the L1495 cloud with…

astro-ph.GA2018

First Data Release of the ESO-ARO Public Survey SAMPLING --- SMT "All-sky" Mapping of PLanck Interstellar Nebulae in the Galaxy

Ke Wang, Sarolta Zahorecz, Maria R. Cunningham +17

We make the first data release (DR1) of the ongoing ESO Public Survey SAMPLING (http://dx.doi.org/10.7910/DVN/0L8NHX). DR1 comprises of 124 fields distributed in $70^\circ < l < 21…