Results 151 to 160 of about 238,168 (251)
We dendrogram the Leike et al. 3D dust map, leveraging its ∼1 pc spatial resolution to produce a uniform catalog of molecular clouds in the solar neighborhood. Using accurate distances, we measure the properties of 65 clouds in true 3D space, eliminating
Shlomo Cahlon+4 more
doaj +1 more source
Oxygen fractionation in dense molecular clouds. [PDF]
Loison JC+15 more
europepmc +1 more source
Effects of grain alignment efficiency on synthetic dust polarization observations of molecular clouds. [PDF]
King PK, Chen CY, Fissel LM, Li ZY.
europepmc +1 more source
On the redistribution of OB star luminosity and the warming of nearby molecular clouds [PDF]
Infrared Astronomy Satellite (IRAS) observations of the neighborhoods of six outer-Galaxy HII regions were combined with CO observations to show that most of the far infrared (FIR) luminosity from within approximately 25 to 75 pc of the ionizing stars is
Leisawitz, D.
core +1 more source
The Evolution of Molecular Clouds: Turbulence-regulated Global Radial Collapse
The star formation efficiency (SFE) measures the proportion of molecular gas converted into stars, while the star formation rate (SFR) indicates the rate at which gas is transformed into stars.
An-Xu Luo, Hong-Li Liu, Jin-Zeng Li
doaj +1 more source
Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback. [PDF]
Kruijssen JMD+9 more
europepmc +1 more source
The detection of the J = 3-2 lines of HCN, HNC, and HCO/+/ in the Orion molecular cloud
P. J. Huggins+5 more
openalex +1 more source
Gas phase Elemental abundances in Molecular cloudS (GEMS): I. The prototypical dark cloud TMC 1. [PDF]
Fuente A+32 more
europepmc +1 more source