P Girichidis, SSR Offner, AG Kritsuk, RS Klessen… - Space Science …, 2020 - Springer
Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy …
J Sun, AK Leroy, E Rosolowsky, A Hughes… - The Astronomical …, 2022 - iopscience.iop.org
We present a rich, multiwavelength, multiscale database built around the PHANGS–ALMA CO (2− 1) survey and ancillary data. We use this database to present the distributions of …
V Könyves, P André, A Men'Shchikov… - Astronomy & …, 2015 - aanda.org
We present and discuss the results of the Herschel Gould Belt survey (HGBS) observations in an~ 11 deg 2 area of the Aquila molecular cloud complex at d~ 260 pc, imaged with the …
J Sun, AK Leroy, EC Ostriker, S Meidt… - The Astrophysical …, 2023 - iopscience.iop.org
We measure empirical relationships between the local star formation rate (SFR) and properties of the star-forming molecular gas on 1.5 kpc scales across 80 nearby galaxies …
EC Ostriker, CG Kim - The Astrophysical Journal, 2022 - iopscience.iop.org
The star formation rate (SFR) in galactic disks depends on both the quantity of the available interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …
Understanding the physics of turbulence is crucial for many applications, including weather, industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …
JG Kim, EC Ostriker, N Filippova - The Astrophysical Journal, 2021 - iopscience.iop.org
Molecular clouds are supported by turbulence and magnetic fields, but quantifying their influence on cloud life cycle and star formation efficiency (SFE) remains an open question …
We address the problem of the origin of massive stars, namely the origin, path, and timescale of the mass flows that create them. Based on extensive numerical simulations, we …
ABSTRACT After two Atacama Large Millimeter/submillimeter Array (ALMA) observing cycles, only a handful of [C ii] 158 μm emission line searches in z> 6 galaxies have reported …