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Ionized-gas

Tracing kinematic (mis)alignments in CALIFA merging galaxies : Stellar and ionized gas kinematic orientations at every merger stage

Tracing kinematic (mis)alignments in CALIFA merging galaxies : Stellar and ionized gas kinematic orientations at every merger stage

... and ionized gas morpho-kinematic mis- alignments larger than those found in the control ...the ionized gas kinematic PA (66 objects) reveals that 42% (28 / 66) of the interacting sample has ...

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Radiation hydrodynamics simulations of the evolution of the diffuse ionized gas in disc galaxies

Radiation hydrodynamics simulations of the evolution of the diffuse ionized gas in disc galaxies

... Fig. 13 shows line emission maps for the main tracers of the neutral and ionized gas in our discs for different ionizing source luminosities. All of these were created by integrating the contri- butions of ...

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Hall Effects on the Flow of an Ionized Gas between a Parallel Flat Wall and a long Wavy Wall

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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The spatially resolved stellar population and ionized gas properties in the merger LIRG NGC 2623

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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VLT FORS2 optical imaging and spectroscopy of nine luminous type 2 AGN at 0.3 < z < 0.6-I. Ionized gas nebulae

VLT FORS2 optical imaging and spectroscopy of nine luminous type 2 AGN at 0.3 < z < 0.6-I. Ionized gas nebulae

... K) ionized gas are frequently detected ...this gas is dominated by photoionization by the hard radiation field of the central AGN, with an occasional contribution from young stars (Villar-Mart´ın et ...

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1D Kinematics from stars and ionized gas at $z\sim0 8$ from the LEGA C spectroscopic survey of massive galaxies

1D Kinematics from stars and ionized gas at $z\sim0 8$ from the LEGA C spectroscopic survey of massive galaxies

... the ionized gas can have a range of spatial ...by gas inflows and outflows and central AGN ...than gas kinemat- ics (25 with (σ ?,int 0 /σ 0 g,int ) > ...the ionized gas is ...

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The SAMI galaxy survey : kinematics of dusty early type galaxies

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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A jet-induced outflow of warm gas in 3C 293

A jet-induced outflow of warm gas in 3C 293

... emission-line gas (the component that represents the ionized gas outflows) is blueshifted with respect to the narrow component on the eastern side and redshifted on the western side (in the case ...

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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

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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"We Are Not Hired Help:" The 1968 Statewide Florida Teacher Strike, the Rise of Modern Conservatism, and the Potency of Teacher Power

"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 ...

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Comparative Effects of Non Thermal Atmospheric Pressure Plasma on Migration and Invasion in Oral Squamous Cell Cancer, by Gas Type

Comparative Effects of Non Thermal Atmospheric Pressure Plasma on Migration and Invasion in Oral Squamous Cell Cancer, by Gas Type

... Purpose: The fourth state of matter, plasma is known as an ionized gas with electrons, radicals and ions. The use of non-thermal plasma (NTP) in cancer research became possible because of the progresses in ...

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Radiative transfer calculations of the diffuse ionized gas in disc galaxies with cosmic ray feedback

Radiative transfer calculations of the diffuse ionized gas in disc galaxies with cosmic ray feedback

... To perform the post-processing with our radiative trans- fer code, we resample the density grids on a Cartesian grid of 128×128×256 cells, in a box with dimensions 2×2× ±2 kpc, and with the same periodic boundaries as ...

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Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions

Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions

... for ionized gas at ...the ionized gas tends to be associated toward the millimeter clumps; of the 31 millimeter clumps observed, nine of these appear to be physically related to ionized ...

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Transport phenomena in neutral and ionized gases

Transport phenomena in neutral and ionized gases

... accommodate the changes in observed mobilities by alteration of gas density. The purpose of this is to show that the values originally assigned to the parameters are physical. However, it is not suggested that the ...

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Wettability alteration by magnesium ion binding in heavy oil/brine/chemical/sand systems—analysis of hydration forces

Wettability alteration by magnesium ion binding in heavy oil/brine/chemical/sand systems—analysis of hydration forces

... heavy oil (oil/water volume ratio = 1:1), no further re- duction in surface tension of the water phase was ob- served within the experimental error. This suggests that no organic acids in the oil phase partitioned into ...

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Ionized gas discs in elliptical and S0 galaxies at z < 1

Ionized gas discs in elliptical and S0 galaxies at z < 1

... The ETGs considered in this paper are all elliptical and S0 galaxies with no strong signs of interaction or morphological distortions in their HST images. However, to identify the presence of small mor- phological ...

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Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics

Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics

... To investigate the impact of our approximations on the re- sult of the 1D models, we reran our 1D test with the radi- ation hydrodynamics code torus (Harries 2000), using the “detailed” model as described in Haworth et ...

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CIELO-RGS : a catalogue of soft X-ray ionized emission lines

CIELO-RGS : a catalogue of soft X-ray ionized emission lines

... He-α transition derived from the CIELO catalogue for the two soft X-ray brightest heavily ob- scured AGN (NGC 1068, and NGC 4151) (Guainazzi & Bianchi 2007), and for a sample of active stars. Multiple data points for ...

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Linear Waves in Partially Ionized Plasmas in Ionization Non-equilibrium

Linear Waves in Partially Ionized Plasmas in Ionization Non-equilibrium

... Finally, as a third possibility is to deal with this problem by assuming that non-equilibrium effects appear only in the perturbed state (and this is the possibility employed in the present paper). Similar to the ...

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Buoyancy-driven magnetohydrodynamic waves in a partially ionized plasma

Buoyancy-driven magnetohydrodynamic waves in a partially ionized plasma

... fully ionized MHD description valid? In this article, we investigate the effect of partial ionization on buoyancy-driven MHD waves (the MHD analog of internal gravity waves) by applying a simplified two-fluid ...

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