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... • Can one define a metric to indicate whether the necessary physics of the flows of interest have been captured and suitably resolved using the tools available to the researcher? ...
... • Can one define a metric to indicate whether the necessary physics of the flows of interest have been captured and suitably resolved using the tools available to the researcher? ...
Triggered/sequential star formation? A multi
... and classified more than 5000 bubbles. Infrared bubbles are defined by their bright 8 μm emission rims. Although their origin may be manifold, many of the bubbles have shown to be created by a, not necessarily central, ionizing source. In this context, the emission rim originates from UV excited pol ...
... and classified more than 5000 bubbles. Infrared bubbles are defined by their bright 8 μm emission rims. Although their origin may be manifold, many of the bubbles have shown to be created by a, not necessarily central, ionizing source. In this context, the emission rim originates from UV excited pol ...
Rearrangement of gas in disc galaxies
... Observation of disc galaxies confirm the presence of large concentrations of gas in their circumnuclear regions, however, galaxy formation models do not always give rise to the observed central gas concentrations right after the formation process is completed. A corollary of this picture is thus tha ...
... Observation of disc galaxies confirm the presence of large concentrations of gas in their circumnuclear regions, however, galaxy formation models do not always give rise to the observed central gas concentrations right after the formation process is completed. A corollary of this picture is thus tha ...
Matter Cycle in the Interstellar Medium (ISM)
... stars was filled with interstellar gas, transparent in the visible, except for a few spectral lines arising from atomic ground states. (but this could not explain the dark clouds catalogued by Barnard.) Diameter ...
... stars was filled with interstellar gas, transparent in the visible, except for a few spectral lines arising from atomic ground states. (but this could not explain the dark clouds catalogued by Barnard.) Diameter ...
The mid- and far-infrared range - International Space Science Institute
... spectral line) required to achieve a 10 σ detection in 104 s for the different observatories. Detection of wider features depends on the resolution of the instrument. These are for the grating instruments on JWST R ≈ 3000, on Spitzer R ≈ 600, on Gemini R ≈ 200 in N and R ≈ 100 in Q, on ISO R ≈ 1500 ...
... spectral line) required to achieve a 10 σ detection in 104 s for the different observatories. Detection of wider features depends on the resolution of the instrument. These are for the grating instruments on JWST R ≈ 3000, on Spitzer R ≈ 600, on Gemini R ≈ 200 in N and R ≈ 100 in Q, on ISO R ≈ 1500 ...
813. - Materials and Process Simulation Center
... ReaxFF leads to a plausible description of hydrazine thermal decomposition. Our results show that the primary reaction product of hydrazine decomposition is NH3, which at elevated temperatures is converted into the entropically more favorable H2 and N2. 4.1.3. Reaction Mechanism. To accurately model ...
... ReaxFF leads to a plausible description of hydrazine thermal decomposition. Our results show that the primary reaction product of hydrazine decomposition is NH3, which at elevated temperatures is converted into the entropically more favorable H2 and N2. 4.1.3. Reaction Mechanism. To accurately model ...
Absence of Metallization in Solid Molecular Hydrogen
... at variance to the semilocal DFT results and eventually entails an even higher metallization pressure. In general, except for the Cmca-12 structure, which up to ∼375 GPa is more stable than expected, the aforementioned rule of Kaxiras et al. is very well maintained at the hybrid DFT level. In partic ...
... at variance to the semilocal DFT results and eventually entails an even higher metallization pressure. In general, except for the Cmca-12 structure, which up to ∼375 GPa is more stable than expected, the aforementioned rule of Kaxiras et al. is very well maintained at the hybrid DFT level. In partic ...
Media Alert A new spin on star-forming galaxies
... “We see that galaxy the way it probably looks now… something could have happened to it but it’s very unlikely,” he said. “The galaxies that are 10 billion light years away, that’s comparable to a picture from when you were three or four years old, that’s very different.” The team used the Keck and G ...
... “We see that galaxy the way it probably looks now… something could have happened to it but it’s very unlikely,” he said. “The galaxies that are 10 billion light years away, that’s comparable to a picture from when you were three or four years old, that’s very different.” The team used the Keck and G ...
Microplasma
Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.