Results 21 to 30 of about 5,519,686 (289)

Molecular thermodynamics of gas solubility [PDF]

open access: yesFluid Phase Equilibria, 1985
A molecular-thermodynamic model has been established for the solubilities of gases in non-polar and polar solvents and in aqueous solutions of electrolytes. To obtain an expression for the Helmholtz energy of the mixture, the pure components are first mixed isothermally to form an ideal gas mixture.
Hu, Y., Xu, Y.N., Prausnitz, J.M.
openaire   +2 more sources

COLD MOLECULAR GAS IN MERGER REMNANTS. I. FORMATION OF MOLECULAR GAS DISKS [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2014
35 pages, 7 figures, 6 tables, accepted for publication in ApJS. For high-quality images and data products (in FITS format), see http://alma-intweb.mtk.nao.ac.jp/~jueda/data/mr/index ...
Junko Ueda   +13 more
openaire   +2 more sources

MODELING THE MOLECULAR GAS IN NGC 6240 [PDF]

open access: yesThe Astrophysical Journal, 2015
We present the first observations of H$^{13}$CN$(1-0)$, H$^{13}$CO$^+(1-0)$ and SiO$(2-1)$ in NGC\,6240, obtained with the IRAM PdBI. Combining a Markov Chain Monte Carlo (MCMC) code with Large Velocity Gradient (LVG) modelling, and with additional data from the literature, we simultaneously fit three gas phases and six molecular species to constrain ...
R. Tunnard   +7 more
openaire   +3 more sources

Sensitive Spectroscopy of Acetone Using a Widely Tunable External-Cavity Quantum Cascade Laser

open access: yesSensors, 2018
We employed a single-mode, widely tunable (~300 cm−1) external-cavity quantum cascade laser operating around 8 µm for broadband direct absorption spectroscopy and wavelength modulation spectroscopy where a modulation frequency of 50 kHz was ...
Faisal Nadeem   +4 more
doaj   +1 more source

Molecular gas toward G18.8+1.8 [PDF]

open access: yesAstronomy & Astrophysics, 2012
This work aims at investigating the characteristics of the molecular gas associated with the nebula G18.8+1.8, linked to the Wolf-Rayet star HD168206 (WR 113), and its relation to other components of its local interstellar medium. We carried out molecular observations of the 12CO(J=1-0) and (J=2-1) lines with angular resolution of 44 arcsec and 22 ...
Vasquez, Javier   +3 more
openaire   +6 more sources

The importance of mean free path in determining gas flow behaviour [PDF]

open access: yes, 2010
We investigate whether a power-law form of probability distribution function better describes the free paths of dilute gas molecules in a confined system.
Dongari, Nishanth   +5 more
core   +5 more sources

The State of the Molecular Gas in Post-starburst Galaxies

open access: yesThe Astrophysical Journal, 2023
The molecular gas in galaxies traces both the fuel for star formation and the processes that can enhance or suppress star formation. Observations of the molecular gas state can thus point to when and why galaxies stop forming stars.
K. Decker French   +9 more
doaj   +1 more source

Molecular Gas in Galactic Nuclei [PDF]

open access: yesHighlights of Astronomy, 1989
Recent high resolution interferometric observations of the molecular gas in luminous IR galaxies reveal extraordinary concentrations of star forming material in the central few kpc. In several of the nearest IR bright galaxies, the molecular gas in the central regions is concentrated in a bar-like distribution (IC342, NGC 6946, and NGC 253) and in NGC ...
openaire   +1 more source

The molecular gas mass of M 33 [PDF]

open access: yesAstronomy & Astrophysics, 2017
Do some environments favor efficient conversion of molecular gas into stars? To answer this, we need to be able to estimate the H2 mass. Traditionally, this is done using CO observations and a few assumptions but the Herschel observations which cover the far-IR dust spectrum make it possible to estimate the molecular gas mass independently of CO and ...
Gratier, P.   +17 more
openaire   +6 more sources

The molecular gas distribution in M51

open access: yesThe Astrophysical Journal, 1983
CO emission has been mapped along four strips in M51 using the 14 m Five College Radio Astronomy Observatory telescope (HPBW = 50'') in order to sample the radial distribution of molecular gas. The derived abundance of H/sub 2/ shows that three-fourths of the interstellar medium (ISM) nucleons are in H/sub 2/ rather than H I in the disk at ...
SCOVILLE, N, Young, JS
openaire   +2 more sources

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