Results 141 to 150 of about 22,673 (314)
Unstructured Voronoi mesh simulations offer many advantages for simulating self-gravitating gas dynamics on galactic scales. Adaptive mesh refinement (AMR) can be a powerful tool for simulating the details of star cluster formation and gas dispersal by ...
Sean C. Lewis +7 more
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
Additive manufacturing revolutionizes production by enabling on‐demand, customized, and sustainable manufacturing with streamlined supply chains. While metal and polymer AM are well‐established, advanced ceramic AM is rapidly emerging, overcoming traditional material challenges.
Kateryna Oleksandrivna Shvydyuk +2 more
wiley +1 more source
Molecular hydrogen (H _2 ) formation and dissociation are key processes that drive the gas life cycle in galaxies. Using the SImulating the LifeCycle of Molecular Clouds zoom-in simulation suite, we explore the utility of future observations of H _2 ...
Blakesley Burkhart +13 more
doaj +1 more source
Can The Virial Parameter Reliably Trace The Dynamical State Of Molecular Clouds?
Camilo Peñaloza
openalex +2 more sources
A method to determine distances to molecular clouds using near-IR photometry [PDF]
G. Maheswar +4 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
15 pages, 7 figure files. Invited review for "The Dynamic ISM: A celebration of the Canadian Galactic Plane Survey," ASP Conference Series, from conference held in Naramata BC, Canada June 6-10 ...
openaire +2 more sources
This study demonstrates an aluminum‐based hybrid photoresist synthesized via molecular layer deposition (MLD) using trimethylaluminum and hydroquinone. The resist achieves sub‐20 nm resolution and virtually infinite silicon etch selectivity, enabling 40 nm‐wide, micrometer‐tall nanostructures.
Won‐Il Lee +8 more
wiley +1 more source
High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm [PDF]
Roya Hamedani Golshan +6 more
openalex +1 more source

