Synthetic observations of star formation and the interstellar medium
Synthetic observations are playing an increasingly important role across astrophysics, both
for interpreting real observations and also for making meaningful predictions from models. In …
for interpreting real observations and also for making meaningful predictions from models. In …
Distributed star formation throughout the Galactic Center cloud Sgr B2
A Ginsburg, J Bally, A Barnes, N Bastian… - The Astrophysical …, 2018 - iopscience.iop.org
We report ALMA observations with resolution≈ 0 farcs 5 at 3 mm of the extended Sgr B2
cloud in the Central Molecular Zone (CMZ). We detect 271 compact sources, most of which …
cloud in the Central Molecular Zone (CMZ). We detect 271 compact sources, most of which …
The physical and chemical structure of Sagittarius B2-II. Continuum millimeter emission of Sgr B2 (M) and Sgr B2 (N) with ALMA
Á Sánchez-Monge, P Schilke, A Schmiedeke… - Astronomy & …, 2017 - aanda.org
Context. The two hot molecular cores Sgr B2 (M) and Sgr B2 (N), which are located at the
center of the giant molecular cloud complex Sagittarius B2, have been the targets of …
center of the giant molecular cloud complex Sagittarius B2, have been the targets of …
The physical and chemical structure of Sagittarius B2-IV. Converging filaments in the high-mass cluster forming region Sgr B2 (N)
A Schwörer, Á Sánchez-Monge, P Schilke… - Astronomy & …, 2019 - aanda.org
Context. Sagittarius B2 (north) is a chemically rich, high-mass star-forming region located
within the giant molecular cloud complex Sgr B2 in the central molecular zone of our Galaxy …
within the giant molecular cloud complex Sgr B2 in the central molecular zone of our Galaxy …
Toward gas exhaustion in the W51 high-mass protoclusters
A Ginsburg, WM Goss, C Goddi… - Astronomy & …, 2016 - aanda.org
We present new JVLA observations of the high-mass cluster-forming region W51A from 2 to
16 GHz with resolution θ fwhm≈ 0.3− 0.5 ″. The data reveal a wealth of observational …
16 GHz with resolution θ fwhm≈ 0.3− 0.5 ″. The data reveal a wealth of observational …
Super Hot Cores in NGC 253: witnessing the formation and early evolution of super star clusters
F Rico-Villas, J Martin-Pintado… - Monthly Notices of …, 2020 - academic.oup.com
ABSTRACT Using 0.2 arcsec (∼ 3 pc) ALMA images of vibrationally excited HC3N emission
(HC3N*) we reveal the presence of eight unresolved Super Hot Cores (SHCs) in the inner …
(HC3N*) we reveal the presence of eight unresolved Super Hot Cores (SHCs) in the inner …
Thermal Feedback in the High-mass Star-and Cluster-forming Region W51
A Ginsburg, C Goddi, JMD Kruijssen… - The Astrophysical …, 2017 - iopscience.iop.org
High-mass stars have generally been assumed to accrete most of their mass while already
contracted onto the main sequence, but this hypothesis has not been observationally tested …
contracted onto the main sequence, but this hypothesis has not been observationally tested …
Seeding the Galactic Centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds
JD Henshaw, SN Longmore… - Monthly Notices of the …, 2016 - academic.oup.com
Star formation within the Central Molecular Zone (CMZ) may be intimately linked to the
orbital dynamics of the gas. Recent models suggest that star formation within the dust ridge …
orbital dynamics of the gas. Recent models suggest that star formation within the dust ridge …
Modeling of the effects of stellar feedback during star cluster formation using a hybrid gas and n-body method
JE Wall, MM Mac Low, SLW McMillan… - The Astrophysical …, 2020 - iopscience.iop.org
Understanding the formation of stellar clusters requires following the interplay between gas
and newly formed stars accurately. We therefore couple the magnetohydrodynamics code …
and newly formed stars accurately. We therefore couple the magnetohydrodynamics code …
Physical processes in the interstellar medium
NY Gnedin, SCO Glover, RS Klessen… - Star Formation in Galaxy …, 2016 - Springer
Understanding the physical processes that govern the dynamical behavior of the interstellar
medium (ISM) is central to much of modern astronomy and astrophysics. The ISM is the …
medium (ISM) is central to much of modern astronomy and astrophysics. The ISM is the …