Photodissociation and X-Ray-Dominated Regions
MG Wolfire, L Vallini, M Chevance - Annual Review of …, 2022 - annualreviews.org
The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …
Toward understanding massive star formation
H Zinnecker, HW Yorke - Annu. Rev. Astron. Astrophys., 2007 - annualreviews.org
Although fundamental for astrophysics, the processes that produce massive stars are not
well understood. Large distances, high extinction, and short timescales of critical …
well understood. Large distances, high extinction, and short timescales of critical …
PHANGS–JWST First Results: A Statistical View on Bubble Evolution in NGC 628
The first JWST observations of nearby galaxies have unveiled a rich population of bubbles
that trace the stellar-feedback mechanisms responsible for their creation. Studying these …
that trace the stellar-feedback mechanisms responsible for their creation. Studying these …
The Spitzer/GLIMPSE surveys: a new view of the Milky Way
E Churchwell, BL Babler, MR Meade… - Publications of the …, 2009 - iopscience.iop.org
ABSTRACT A brief description is given of the GLIMPSE surveys, including the areas
surveyed, sensitivity limits, and products. The primary motivations for this review are to …
surveyed, sensitivity limits, and products. The primary motivations for this review are to …
Cloud–cloud collisions and triggered star formation
Star formation is a fundamental process for galactic evolution. One issue over the last
several decades has been determining whether star formation is induced by external …
several decades has been determining whether star formation is induced by external …
Unifying low-and high-mass star formation through density-amplified hubs of filaments-The highest mass stars (> 100 M⊙) form only in hubs
MSN Kumar, P Palmeirim, D Arzoumanian… - Astronomy & …, 2020 - aanda.org
Context. Star formation takes place in giant molecular clouds, resulting in mass-segregated
young stellar clusters composed of Sun-like stars, brown dwarfs, and massive O-type (50 …
young stellar clusters composed of Sun-like stars, brown dwarfs, and massive O-type (50 …
MIPSGAL: A Survey of the Inner Galactic Plane at 24 and 70 μm
ABSTRACT MIPSGAL is a 278 deg 2 survey of the inner Galactic plane using the Multiband
Infrared Photometer for Spitzer aboard the Spitzer Space Telescope. The survey field was …
Infrared Photometer for Spitzer aboard the Spitzer Space Telescope. The survey field was …
The disruption of giant molecular clouds by radiation pressure & the efficiency of star formation in galaxies
Star formation is slow in the sense that the gas consumption time is much longer than the
dynamical time. It is also inefficient; star formation in local galaxies takes place in giant …
dynamical time. It is also inefficient; star formation in local galaxies takes place in giant …
Ionizing feedback from massive stars in massive clusters–II. Disruption of bound clusters by photoionization
JE Dale, B Ercolano, IA Bonnell - Monthly Notices of the Royal …, 2012 - academic.oup.com
We present a smoothed particle hydrodynamics parameter study of the dynamical effect of
photoionization from O-type stars on star-forming clouds of a range of masses and sizes …
photoionization from O-type stars on star-forming clouds of a range of masses and sizes …
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 …