Results 11 to 20 of about 4,469,999 (359)

Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback. [PDF]

open access: yesNature, 2019
The physics of star formation and the deposition of mass, momentum and energy into the interstellar medium by massive stars (‘feedback’) are the main uncertainties in modern cosmological simulations of galaxy formation and evolution1,2.
Kruijssen JMD   +9 more
europepmc   +3 more sources

On the Three-dimensional Structure of Local Molecular Clouds [PDF]

open access: yesAstrophysical Journal, 2021
We leverage the 1 pc spatial resolution of the Leike et al. three-dimensional (3D) dust map to characterize the 3D structure of nearby molecular clouds (d ≲ 400 pc).
C. Zucker   +11 more
semanticscholar   +1 more source

A compendium of distances to molecular clouds in the Star Formation Handbook [PDF]

open access: yesAstronomy & Astrophysics, 2020
Accurate distances to local molecular clouds are critical for understanding the star and planet formation process, yet distance measurements are often obtained inhomogeneously on a cloud-by-cloud basis.
C. Zucker   +6 more
semanticscholar   +1 more source

A large catalogue of molecular clouds with accurate distances within 4 kpc of the Galactic disc [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
We present a large, homogeneous catalogue of molecular clouds within 4 kpc from the Sun at low Galactic latitudes (|b| 
B.-Q. Chen   +8 more
semanticscholar   +1 more source

Distances and Statistics of Local Molecular Clouds in the First Galactic Quadrant [PDF]

open access: yesAstrophysical Journal, 2020
We present an analysis of local molecular clouds ( km s−1, i.e.,
Q. Yan   +4 more
semanticscholar   +1 more source

The SEDIGISM survey: molecular clouds in the inner Galaxy [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2020
We use the 13CO (2–1) emission from the SEDIGISM (Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium) high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic ...
A. Duarte-Cabral   +59 more
semanticscholar   +1 more source

A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition [PDF]

open access: yesAstrophysical Journal, 2019
We present a uniform catalog of accurate distances to local molecular clouds informed by the Gaia DR2 data release. Our methodology builds on that of Schlafly et al.
C. Zucker   +6 more
semanticscholar   +1 more source

CO TO H2 RATIO OF INTERSTELLAR MOLECULAR CLOUDS IN THE DIRECTIONS OF EARLY TYPE STARS [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2004
We present measurements of interstellar CO absorption lines in the spectra of 7 early-type stars that were observed with the FUSE(Far Ultraviolet Spectroscopic Explorer).
Jae-Woo Park   +2 more
doaj   +1 more source

Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
We present a unified description of the scenario of global hierarchical collapse (GHC). GHC constitutes a flow regime of (non-homologous) collapses within collapses, in which all scales accrete from their parent structures, and small, dense regions begin
E. V'azquez-Semadeni   +4 more
semanticscholar   +1 more source

Turbulence in Molecular Clouds [PDF]

open access: yesThe Astrophysical Journal, 1995
accepted in ApJ, compressed postscript, figures not included. Complete preprint available at http://ucowww.ucsc.edu/~dubinski/home.html or by request to dubinski@lick.ucsc ...
John Dubinski   +2 more
openaire   +4 more sources

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