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[PDF] Top 20 Physical properties of dense molecular gas in centres of Seyfert galaxies

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Physical properties of dense molecular gas in centres of Seyfert galaxies

Physical properties of dense molecular gas in centres of Seyfert galaxies

... data of the dense molecular gas in the central 50–100 pc of four nearby Seyfert ...observations of HCN and, in two of the four sources, simultaneously ... Voir le document complet

14

Thick discs, and an outflow, of dense gas in the nuclei of nearby Seyfert galaxies

Thick discs, and an outflow, of dense gas in the nuclei of nearby Seyfert galaxies

... variety of sources and methods, Hicks et ...typical gas mass fraction lies in the range 4–25 per cent, with a typical value of f gas ∼ ...the centres of AGN since it would ... Voir le document complet

18

The ATLAS3D project - XI. Dense molecular gas properties of CO-luminous early-type galaxies

The ATLAS3D project - XI. Dense molecular gas properties of CO-luminous early-type galaxies

... 3. Molecular line ratio diagrams. Early-type galaxies are represented by yellow squares with error bars or upper or lower ...and Seyfert nuclei are portrayed by purple circles, green stars and blue ... Voir le document complet

19

Robust prediction of dense gas flows under uncertain thermodynamic models

Robust prediction of dense gas flows under uncertain thermodynamic models

... BMSA). In this case the models are weighted by their posterior probabilities (resulting from inference on a given scenario) while the scenarios are assigned a prior probability mass function based on the level ... Voir le document complet

23

Small-scale dynamics of dense gas compressible homogeneous isotropic turbulence

Small-scale dynamics of dense gas compressible homogeneous isotropic turbulence

... of energy exchanges. Furthermore, the probability distribution of local dilatation was shown to develop long negative tails (thus leading to a negative ...skewness). In a previous paper, the present ... Voir le document complet

36

ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments

ALMA Observations of Gas-rich Galaxies in z ~ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments

... detections in 11 gas-rich cluster galaxies at ...sample of molecular gas measurements in z ...Adaptation of the Red-sequence Cluster Survey. We augment the >5σ ... Voir le document complet

7

Properties of Faint Distant Galaxies as seen through Gravitational Telescopes

Properties of Faint Distant Galaxies as seen through Gravitational Telescopes

... One of the main possible applications of GTs is the research and study of the very first stars and galaxies forming from pristine matter in the early Universe, the so-called Population ... Voir le document complet

27

The formation of dense gas in low- and high-mass star forming regions

The formation of dense gas in low- and high-mass star forming regions

... filaments in the ISM were known since long, it was the unprecedented sensitivity of the Her- schel telescope that highlighted the ubiquitous filamentary nature of the dense ISM in ... Voir le document complet

237

Observation of magneto-electric non-reciprocity in molecular nitrogen gas

Observation of magneto-electric non-reciprocity in molecular nitrogen gas

... quality of the alignment and the cleanliness of the mirrors, resulting in a cavity linewidth (FWHM) between 13 and 4 ...linewidth of 5 kHz in 1 ms) is injected in both clockwise ... Voir le document complet

5

HyperLabels---Browsing of Dense and Hierarchical Molecular 3D Models

HyperLabels---Browsing of Dense and Hierarchical Molecular 3D Models

... kind of abstract data that is usually visualized using abstract visual ...arrangement of structures as well as concentrations and distributions of each elementary building type in ...aspect ... Voir le document complet

13

The ARGOS Wavefront Sensor Detector and Computer and The Black Hole Growth of Narrow-Line Seyfert 1 Galaxies

The ARGOS Wavefront Sensor Detector and Computer and The Black Hole Growth of Narrow-Line Seyfert 1 Galaxies

... discussed in the last section 5.4.3, the radiative efficiency of the AGNs have a direct impact on their black hole growth and their final black hole ...which in turn is influenced by the AGN ... Voir le document complet

223

Dense gas effects in inviscid homogeneous isotropic turbulence

Dense gas effects in inviscid homogeneous isotropic turbulence

... study of the influence of dense gas effects on the large-scale dynamics of decaying homogeneous isotropic turbulence is carried out by using the van der Waals gas ...on ... Voir le document complet

41

Role of Physical Bolus Properties as Sensory Inputs in the Trigger of Swallowing

Role of Physical Bolus Properties as Sensory Inputs in the Trigger of Swallowing

... Portions of 3 g of petal wheat-flake cereals were prepared before each session and presented to the subject in a ...time of spontaneous swallowing under experimental ...Number of cycles ... Voir le document complet

9

Survey of the Physical Properties of Hollow Concrete Blocks Produced in Canada

Survey of the Physical Properties of Hollow Concrete Blocks Produced in Canada

... A survey of concrete block production was undertaken because of a need for information on the composition, shape and size of hollow.. concrete blocks produced in Canada.[r] ... Voir le document complet

20

A design space of guidance techniques for large and dense physical environments

A design space of guidance techniques for large and dense physical environments

... scope of Buchmann et ...representation of the design space shown in Figure 1 describes techniques in terms of modality, physicality, type, and granularity in a way that helps to ... Voir le document complet

10

Molecular simulation of gas adsorption, diffusion, and permeation in hydrated Nafion membranes

Molecular simulation of gas adsorption, diffusion, and permeation in hydrated Nafion membranes

... isotherms of gases in the hydrated Nafion membrane can be obtained using Henry constant calcu- lated from excess chemical potentials, as shown in eq ...amount of gas molecules follows ... Voir le document complet

8

A design space of guidance techniques for large and dense physical environments

A design space of guidance techniques for large and dense physical environments

... object in a physical environment is difficult if the environment contains many objects, especially if it is large and ...using physical objects or virtual ...vicinity of the target or to ... Voir le document complet

10

On the physical properties of poly(ethylene 2,5-furandicarboxylate)

On the physical properties of poly(ethylene 2,5-furandicarboxylate)

... 3.2 PROPERTIES OF ORIENTED SAMPLES CRYSTALLINITY AND SHRINKAGE DSC measurements were performed on the oriented PEF and PET samples in order to investigate the development of strain induced ... Voir le document complet

203

Influence of the sintering atmosphere on dense Uranium mono-carbide properties

Influence of the sintering atmosphere on dense Uranium mono-carbide properties

... investigated in order to obtain a dense, single phase uranium carbide material after ...manufacturing of uranium mono-carbide requires the development of adapted equipment and the use ... Voir le document complet

19

Frequency and properties of bars in cluster and field galaxies at intermediate redshifts

Frequency and properties of bars in cluster and field galaxies at intermediate redshifts

... number of objects studied is small, this is a remarkable ...presence of these large bars at the cluster centers to the interactions proposed to in- stigate bar formation? One plausible scenario would ... Voir le document complet

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