Results 81 to 90 of about 4,796,716 (321)

Co-creation environment with cloud virtual reality and real-time artificial intelligence toward the design of molecular robots

open access: yesJournal of Integrative Bioinformatics, 2022
This paper describes the design philosophy for our cloud-based virtual reality (VR) co-creation environment (CCE) for molecular modeling. Using interactive VR simulation can provide enhanced perspectives in molecular modeling for intuitive live ...
Konagaya Akihiko   +2 more
doaj   +1 more source

QUANTIFYING OBSERVATIONAL PROJECTION EFFECTS USING MOLECULAR CLOUD SIMULATIONS [PDF]

open access: yes, 2013
The physical properties of molecular clouds are often measured using spectral-line observations, which provide the only probes of the clouds' velocity structure.
Christopher Beaumont   +4 more
semanticscholar   +1 more source

Advancing Research on Biomaterials and Biological Materials with Scanning Electron Microscopy under Environmental and Low Vacuum Conditions

open access: yesAdvanced Engineering Materials, EarlyView.
Herein, environmental scanning electron microscopy (ESEM) is discussed as a powerful extension of conventional SEM for life sciences. By combining high‐resolution imaging with variable pressure and humidity, ESEM allows the analysis of untreated biological materials, supports in situ monitoring of hydration‐driven changes, and advances the functional ...
Jendrian Riedel   +6 more
wiley   +1 more source

Molecules in G1.6-0.025 - 'Hot' Chemistry in the Absence of Star Formation at the Periphery of the Galactic Center Region [PDF]

open access: yes, 2009
We present molecular line mapping of the Giant Molecular Cloud G1.6-0.025, which is located at the high longitude end of the Central Molecular Zone of our Galaxy.
Bachiller   +51 more
core   +1 more source

CO abundance variations in the Orion Molecular Cloud [PDF]

open access: yes, 2013
Infrared stellar photometry from the Two Micron All Sky Survey (2MASS) and spectral line imaging observations of 12 CO and 13 CO J = 1-0 line emission from the Five College Radio Astronomy Observatory (FCRAO) 14m telescope are analysed to assess the ...
F. Ripple   +4 more
semanticscholar   +1 more source

Enhancing Low‐Temperature Performance of Sodium‐Ion Batteries via Anion‐Solvent Interactions

open access: yesAdvanced Functional Materials, EarlyView.
DOL is introduced into electrolytes as a co‐solvent, increasing slat solubility, ion conductivity, and the de‐solvent process, and forming an anion‐rich solvent shell due to its high interaction with anion. With the above virtues, the batteries using this electrolyte exhibit excellent cycling stability at low temperatures. Abstract Sodium‐ion batteries
Cheng Zheng   +7 more
wiley   +1 more source

A study of X-ray point sources in Heiles Clouds 1 and 2

open access: yesActa Polytechnica
Star formation takes place in the coldest parts of molecular clouds, beginning in the densest, collapsing regions of filaments. As pre-main sequence stars are luminous X-ray emitters, X-ray point sources can serve as effective tracers of YSOs.
Nóra Varga   +2 more
doaj   +1 more source

Cloud Computing Enabled Big Multi-Omics Data Analytics

open access: yesBioinformatics and Biology Insights, 2021
High-throughput experiments enable researchers to explore complex multifactorial diseases through large-scale analysis of omics data. Challenges for such high-dimensional data sets include storage, analyses, and sharing.
Saraswati Koppad   +3 more
doaj   +1 more source

A CO Line and Infrared Continuum Study of the Active Star-Forming Complex W51

open access: yes, 2010
We present the results of an extensive observational study of the active star-forming complex W51 that was observed in the J=2-1 transition of the 12CO and 13CO molecules over a 1.25 deg x 1.00 deg region with the University of Arizona Heinrich Hertz ...
Arnal   +49 more
core   +1 more source

Excitation and Disruption of a Giant Molecular Cloud by the Supernova Remnant 3C391 [PDF]

open access: yes, 1998
Using the IRAM 30-m telescope, we observed the supernova remnant 3C 391 (G31.9+0.0) and its surroundings in the CO(2-1), HCO+(1-0), CS(2-1), CS(3-2), and CS(5-4) lines.
Downes D.   +10 more
core   +2 more sources

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