Untangling the galaxy. I. Local structure and star formation history of the milky way
Gaia DR2 provides unprecedented precision in measurements of the distance and
kinematics of stars in the solar neighborhood. Through applying unsupervised machine …
kinematics of stars in the solar neighborhood. Through applying unsupervised machine …
A guided map to the spiral arms in the galactic disk of the Milky Way
JP Vallée - Astronomical Review, 2017 - Taylor & Francis
An up-to-date overview of the recent history is given, aiming is to present a helpful working
guide to the literature and at the same time introduce key systems and observational results …
guide to the literature and at the same time introduce key systems and observational results …
FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). I. Project overview and initial results
T Umemoto, T Minamidani, N Kuno… - Publications of the …, 2017 - academic.oup.com
The FUGIN project is one of legacy projects using a new multi-beam FOREST (four-beam
receiver system on the 45 m telescope). This project aims to simultaneously investigate the …
receiver system on the 45 m telescope). This project aims to simultaneously investigate the …
PHANGS–JWST First Results: Tracing the Diffuse Interstellar Medium with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies
KM Sandstrom, EW Koch, AK Leroy… - The Astrophysical …, 2023 - iopscience.iop.org
JWST observations of polycyclic aromatic hydrocarbon (PAH) emission provide some of the
deepest and highest resolution views of the cold interstellar medium (ISM) in nearby …
deepest and highest resolution views of the cold interstellar medium (ISM) in nearby …
The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
RJ Smith, RG Treß, MC Sormani… - Monthly Notices of …, 2020 - academic.oup.com
We introduce a new suite of simulations,'The Cloud Factory', which self-consistently forms
molecular cloud complexes at high enough resolution to resolve internal substructure (up to …
molecular cloud complexes at high enough resolution to resolve internal substructure (up to …
PHANGS–JWST First Results: The Dust Filament Network of NGC 628 and Its Relation to Star Formation Activity
DA Thilker, JC Lee, S Deger, AT Barnes… - The Astrophysical …, 2023 - iopscience.iop.org
Abstract PHANGS–JWST mid-infrared (MIR) imaging of nearby spiral galaxies has revealed
ubiquitous filaments of dust emission in intricate detail. We present a pilot study to …
ubiquitous filaments of dust emission in intricate detail. We present a pilot study to …
Ubiquitous velocity fluctuations throughout the molecular interstellar medium
JD Henshaw, JMD Kruijssen, SN Longmore… - Nature …, 2020 - nature.com
The density structure of the interstellar medium determines where stars form and release
energy, momentum and heavy elements, driving galaxy evolution,,–. Density variations are …
energy, momentum and heavy elements, driving galaxy evolution,,–. Density variations are …
SILCC-Zoom: the dynamic and chemical evolution of molecular clouds
D Seifried, S Walch, P Girichidis, T Naab… - Monthly Notices of …, 2017 - academic.oup.com
We present 3D 'zoom-in'simulations of the formation of two molecular clouds out of the
galactic interstellar medium. We model the clouds–identified from the SILCC simulations …
galactic interstellar medium. We model the clouds–identified from the SILCC simulations …
Large-scale filaments associated with Milky Way spiral arms
K Wang, L Testi, A Ginsburg… - Monthly Notices of …, 2015 - academic.oup.com
The ubiquity of filamentary structure at various scales throughout the Galaxy has triggered a
renewed interest in their formation, evolution, and role in star formation. The largest …
renewed interest in their formation, evolution, and role in star formation. The largest …
The HI/OH/Recombination line survey of the inner Milky Way (THOR)-Survey overview and data release 1
H Beuther, S Bihr, M Rugel, K Johnston… - Astronomy & …, 2016 - aanda.org
Context. The past decade has witnessed a large number of Galactic plane surveys at
angular resolutions below 20′′. However, no comparable high-resolution survey exists at …
angular resolutions below 20′′. However, no comparable high-resolution survey exists at …