ionized gas
Radiation hydrodynamics simulations of the evolution of the diffuse ionized gas in disc galaxies
... of ionized material in our Galaxy was first proposed by Hoyle & Ellis (1963) to explain an ob- served absorption feature in the galactic synchrotron ...warm ionized medium (WIM) (Haffner et ...diffuse ...
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A study of nonlinear phenomena in the propagation of electromagnetic waves in a weakly ionized gas
... When wave form distortion and harmonic wave generation in the two weak transmitted waves due to the effects of nonlinear phenomena in the nonlinear ionized gas are taken into account, th[r] ...
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The spatially resolved stellar population and ionized gas properties in the merger LIRG NGC 2623
... those for two early-stage merger LIRGs (IC 1623 W and NGC 6090), together with CALIFA Sbc/Sc galaxies. We find that NGC 2623 went through two periods of increased star formation (SF), a first and widespread episode, ...
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The Ionized Gas in Nearby Galaxies as Traced by the [N II] 122 and 205 μm Transitions
... One of our main goals is to understand the variations in the ionized gas density as a function of the ISM environment. This is possible thanks to the spatial coverage of our target galaxies provided by ...
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Ionized gas kinematics of galaxies in the CALIFA survey : I Velocity fields, kinematic parameters of the dominant component, and presence of kinematically distinct gaseous systems
... of ionized gas was ob- tained by integrating the signal in the spectral ranges se- lected to apply the CC ...integrated ionized gas kinematics of the galaxies in our sample (see Table ...
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Ionized gas discs in elliptical and S0 galaxies at z < 1
... extended, ionized-gas emission of 24 early-type galaxies (ETGs) at 0 < z < 1 from the ESO Distant Cluster Survey ...disturbed gas kinematics, while 14 have rotating gas ...the gas ...
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Hall Effects on the Flow of an Ionized Gas between a Parallel Flat Wall and a long Wavy Wall
... Abstract: Hall effects on the hydro magnetic flow of an ionized gas between a parallel flat wall and a long wavy wall have been studied. The analytical solution has been derived for velocity distribution. ...
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Weber, Johann Andreas (2018): Three-dimensional, time-dependent radiative transfer for H II regions, the diffuse ionized gas, and the reionization of the universe. Dissertation, LMU München: Fakultät für Physik
... In the present phase of the universe the number and mass fraction of hot massive stars is small com- pared to the total stellar population; however, the impact of these objects on their environment is decisive for the ...
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Jet-driven outflows of ionized gas in the nearby radio galaxy 3C 293
... ionised gas were detected associated with the eastern radio ...ionised gas outflows were remarkably similar and it was therefore concluded that the HI outflows were associated with the same jet-ISM ...
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Radiative transfer calculations of the diffuse ionized gas in disc galaxies with cosmic ray feedback
... The results of these simulations are shown in Fig. 11. As expected, the lower luminosities lead to more noisy tem- perature and Hα profiles, as the sources are no longer able to ionise the entire low density disc. ...
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The peculiar nebula Simeis 57. I. Ionized gas and dust extinction
... In Fig. 9 we compare, in detail, the central parts of the opti- cal and radio images of Simeis 57. The close similiarity is not surprising. On the red PSS image, most of the nebular emis- sion is expected to be a ...
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Energy transfer processes in a partially ionized gas
... Since both representations will, be used in later sections, a general relation between the gradient of the chemical potential and the gradient of the logrrsitlun of the partial pressure [r] ...
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Measurement of the Complex Conductivity of an Ionized Gas at Microwave Frequencies
... As shown below, measurement of these three quantities- effective Q, change in transmission, and change in resonant frequency with discharge currentsuffices to determine both real and ima[r] ...
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"We Are Not Hired Help:" The 1968 Statewide Florida Teacher Strike, the Rise of Modern Conservatism, and the Potency of Teacher Power
... We adopted a Milky Way Galactic extinction curve (Savage & Mathis 1979; Cardelli et al. 1989) to correct the observed emission line ratios that were used to model the ionized gas mass. This assumes that ...
202
Vol 9, No 2 (2018)
... an ionized gas under varied conditions and of different geometrical considerations in slip flow regime represent an area of rapid growth in the contemporary research, but still, there is a few problems ...
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A jet-induced outflow of warm gas in 3C 293
... of ionized gas that is overrun by the lobe of an expanding radio ...the gas gets locked up in these dense fragments that can survive for a long time and reach speeds of up to 500 km s −1 ...
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The SAMI galaxy survey : kinematics of dusty early type galaxies
... and ionized gas kinematics of dusty ETGs using integral field spectroscopy observations from the SAMI Galaxy Survey, and integrated star formation rates, stellar masses and dust masses from the GAMA ...and ...
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Herschel Planetary Nebula Survey (HerPlaNS): hydrogen recombination laser lines in Mz 3
... thin ionized gas, as would be typical for nebular gas in PNe; (ii) the compact core of Mz 3 is responsible for a large fraction of the Herschel HRLs emission; (iii) the line intensity ratios for Mz 3 ...
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The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728
... of ionized gas emission, we find elevated velocities reaching +/- 400 km s − 1 ...detected ionized emission lines show high velocities along the major axis of the NLR and dispersions reaching over ...
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Thesis
... Accurate extraction of rotation curves is vital to ac- complishing the goals of RESOLVE. Optical rotation curves are useful for identifying kinematic anomalies such as non-circular motions and disturbances in the ...
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