activity
20062022
most citedVariations in the Galactic star formation rate and density thresholds for star formation

359 citations · 2.3k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph.GA2022★ 7 cited

Discovery of ammonia (9,6) masers in two high-mass star-forming regions

Y. T. Yan, C. Henkel, K. M. Menten +8

Molecular maser lines are signposts of high-mass star formation, probing excitation and kinematics of very compact regions in the close environment of young stellar objects and pro…

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-ph.GA2021

Clustered Star Formation in the center of NGC 253 Contributes to Driving the Ionized Nuclear Wind

E. A. C. Mills, M. Gorski, K. L. Emig +12

We present new 3 mm observations of the ionized gas toward the nuclear starburst in the nearby (D ~ 3.5 Mpc) galaxy NGC 253. With ALMA, we detect emission from the H40-alpha and He…

astro-ph.GA2021

Physical Conditions in the LMC's Quiescent Molecular Ridge: Fitting Non-LTE Models to CO Emission

Molly K. Finn, Remy Indebetouw, Kelsey E. Johnson +8

The Molecular Ridge in the LMC extends several kiloparsecs south from 30 Doradus, and it contains ~30% of the molecular gas in the entire galaxy. However, the southern end of the M…

astro-ph.GA2020★ 46 cited

Super Star Clusters in the Central Starburst of NGC 4945

Kimberly L. Emig, Alberto D. Bolatto, Adam K. Leroy +12

NGC 4945 is a nearby (3.8 Mpc) galaxy hosting a nuclear starburst and Seyfert Type 2 AGN. We use the Atacama Large Millimeter/submillimeter Array (ALMA) to image the 93 GHz (3.2 mm…

astro-ph.GA2020★ 18 cited

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…