Results 71 to 80 of about 3,373,419 (307)
Molecular cloud dispersal traced by the ionized carbon 158 μm line
Astronomy & AstrophysicsFeedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Not only can feedback compress gas and trigger the formation of dense cores that eventually collapse into new stars, it can also disperse cloud ...
Bonne L. +16 more
doaj +1 more source
RETHINKING A MYSTERIOUS MOLECULAR CLOUD [PDF]
The Astrophysical Journal, 2015 Accepted for publication in ApJ. 16 pages, 13 figures.
openaire +2 more sources
Saint Cloud Reporter [Autumn 1967] [PDF]
, 1967 Saint Cloud Reporter, Autumn 1967https://repository.stcloudstate.edu/magazines/1118/thumbnail ...
St. Cloud State University
core
Inside Dropbox: Understanding Personal Cloud Storage Services [PDF]
, 2012 Personal cloud storage services are gaining popularity. With a rush of providers to enter the market and an increasing of- fer of cheap storage space, it is to be expected that cloud storage will soon generate a high amount of Internet traffic.
Aiko Pras +13 more
core +2 more sources
Advanced Healthcare Materials, EarlyView.The collagen nanofiber (CNF) gel supports cancer cell culture, exhibiting cell morphology and cancer‐related protein expression similar to Matrigel. It offers a higher collagen concentration than commercial gels. Additionally, the CNF gel allows replication of the high elasticity of in vivo cancer tissue by controlling collagen fiber sizes, ranging ...
Naoko Sasaki +4 more
wiley +1 more source
An S-shaped Filament Formed Due to Cloud–Cloud Collision in Molecular Cloud G178.28-00.61
The Astrophysical Journal Supplement SeriesWe present compelling observational evidence supporting G178.28-00.61 as an early-stage candidate for cloud–cloud collision (CCC), with indications of the formation of an S-shaped filament, evenly separated dense cores, and young star clusters.
Tianwei Zhang +20 more
doaj +1 more source
Outer-Galaxy molecular clouds [PDF]
Symposium - International Astronomical Union, 1985 Since our original report of CO emission from outside the solar circle in the first quadrant (Kutner and Mead, 1981) we have extended the observations in two ways: (1) We have improved latitude and longitude coverage. Preliminary results on the latitude distribution were reported by Kutner (1983).
Marc L. Kutner, Kathryn N. Mead
openaire +1 more source
Saint Cloud Reporter [Winter 1967] [PDF]
, 1967 Saint Cloud Reporter, Winter 1967https://repository.stcloudstate.edu/magazines/1117/thumbnail ...
St. Cloud State University
core
Advanced Materials, EarlyView.AI‐Assisted Workflow for (Scanning) Transmission Electron Microscopy: From Data Analysis Automation to Materials Knowledge Unveiling. Abstract (Scanning) transmission electron microscopy ((S)TEM) has significantly advanced materials science but faces challenges in correlating precise atomic structure information with the functional properties of ...
Marc Botifoll +19 more
wiley +1 more source
The Astrophysical JournalMolecular 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