scholarly journals Economic Evaluation of Umeclidinium/Vilanterol versus Umeclidinium or Salmeterol in Symptomatic Non-Exacerbating Patients with COPD from a UK Perspective Using the GALAXY Model

2021 ◽  
Vol Volume 16 ◽  
pp. 3105-3118
Author(s):  
Soham Shukla ◽  
Dhvani Shah ◽  
Alan Martin ◽  
Nancy A Risebrough ◽  
Robyn Kendall ◽  
...  
Keyword(s):  
Economic Evaluation ◽  
The Galaxy ◽  
Galaxy Model

scholarly journals PRS57 - ECONOMIC EVALUATION OF SINGLE INHALER TRIPLE THERAPY FOR PATIENTS WITH CHRONIC OBSTRUCTIVE PULMONARY DISEASE (COPD) USING THE GALAXY MODEL

2018 ◽  
Vol 21 ◽  
pp. S414
Author(s):  
N. Risebrough ◽  
M. Schroeder ◽  
D. Shah ◽  
E. Goodall ◽  
K. Ndirangu ◽  
...  
Keyword(s):  
Chronic Obstructive Pulmonary Disease ◽  
Economic Evaluation ◽  
Triple Therapy ◽  
Pulmonary Disease ◽  
Chronic Obstructive ◽  
Obstructive Pulmonary Disease ◽  
The Galaxy ◽  
Galaxy Model

PRS10 Economic Evaluation of Umeclidinium/Vilanterol Versus Umeclidinium or Salmeterol in a UK COPD Population at Low Risk of Exacerbations Using the GALAXY Model

2021 ◽  
Vol 24 ◽  
pp. S214
Author(s):  
S. Shukla ◽  
D. Shah ◽  
A. Martin ◽  
N.A. Risebrough ◽  
R. Kendall ◽  
...  
Keyword(s):  
Economic Evaluation ◽  
Low Risk ◽  
The Galaxy ◽  
Galaxy Model

scholarly journals Economic Evaluation of Single Inhaler Triple Therapy For Patients With Chronic Obstructive Pulmonary Disease (COPD) Using The Galaxy Model

2017 ◽  
Vol 20 (9) ◽  
pp. A646 ◽  
Author(s):  
S Zhang ◽  
D Shah ◽  
N Risebrough ◽  
AA Martin ◽  
A Briggs ◽  
...  
Keyword(s):  
Chronic Obstructive Pulmonary Disease ◽  
Economic Evaluation ◽  
Triple Therapy ◽  
Pulmonary Disease ◽  
Chronic Obstructive ◽  
Obstructive Pulmonary Disease ◽  
The Galaxy ◽  
Galaxy Model

Modeling the Evolution of Disk Galaxies. I. The Chemodynamical Method and the Galaxy Model

1997 ◽  
Vol 476 (2) ◽  
pp. 544-559 ◽  
Author(s):  
M. Samland ◽  
G. Hensler ◽  
Ch. Theis
Keyword(s):  
Disk Galaxies ◽  
The Galaxy ◽  
Galaxy Model

The Dynamics of Globular Cluster Systems

1988 ◽  
Vol 126 ◽  
pp. 641-642
Author(s):  
Natarajan Ramamani
Keyword(s):  
Gravitational Field ◽  
Globular Cluster ◽  
Cluster System ◽  
Spherically Symmetric ◽  
Cluster Systems ◽  
The Galaxy ◽  
Galaxy Model ◽  
Globular Cluster System ◽  
Hubble Time

This paper describes a project whose aim is to study the dynamics of a globular cluster system using an N-body code modified to include the gravitational field of an isothermal galaxy model. The galaxy and the globular cluster system have the same radii, are spherically symmetric and non-rotating. The evolution is to be followed up to a Hubble time.

scholarly journals 11.16. On the origin of density cusp in galactic nuclei by central black hole

1998 ◽  
Vol 184 ◽  
pp. 487-488
Author(s):  
T. Nakano ◽  
T. Fukushige ◽  
J. Makino
Keyword(s):  
Black Hole ◽  
Hubble Space Telescope ◽  
Outer Region ◽  
Elliptical Galaxies ◽  
Heating Process ◽  
Massive Black Hole ◽  
Weak Density ◽  
The Galaxy ◽  
Galaxy Model ◽  
Inner Region

We investigated the dynamical reaction of the central region of galaxies to a falling massive black hole by N-body simulations. As the initial galaxy model, we used an isothermal King model and placed a massive black hole at around the half-mass radius of the galaxy. We found that the central core of the galaxy is destroyed by the heating due to the black hole and a very weak density cusp (ρ ∝ r−α, with α ∼ 0.5) is formed around the center. This result is consistent with recent observations of large elliptical galaxies by Hubble Space Telescope (Lauer et al. 1995; Byun et al. 1996; Gebhardt et al. 1996; Faber et al. 1996; Kormendy et al. 1996). The radius of the weak cusp region is large for large black hole mass. The velocity of the stars become tangentially anisotropic in the inner region, while in the outer region the stars have radially anisotropic velocity dispersion. Our result naturally explains the mechanism of the formation of the weak cusp found in the previous simulations of galaxy merging, and implies that the weak cusp observed in large elliptical galaxies may be formed by the heating process by sinking black holes during merging events.

Simulating the sky for Gaia: the Galaxy model

1999 ◽  
Vol 8 (1) ◽  
Author(s):  
A. Vallenari ◽  
G. Bertelli ◽  
A. Bressan ◽  
C. Chiosi
Keyword(s):  
The Galaxy ◽  
Galaxy Model

scholarly journals Correction to Absolute Proper Motion Using the IAS-Galaxy Model

1990 ◽  
Vol 141 ◽  
pp. 427-429
Author(s):  
Kavan U. Ratnatunga
Keyword(s):  
Reference Frame ◽  
Proper Motion ◽  
Theoretical Models ◽  
Galactic Structure ◽  
Coordinate Frame ◽  
Proper Motions ◽  
Software Interface ◽  
The Galaxy ◽  
Galaxy Model ◽  
Star Catalogs

The IAS-Galaxy model (Ratnatunga, Bahcall and Casertano 1989) is a software interface between theoretical models of the Galaxy and observed kinematic distributions. It has been developed for analysis of many kinematic catalogs to study global galactic structure. In addition, the IASG model can be used to estimate corrections needed to derive absolute parallax and absolute proper motion by evaluating, on a star-by-star basis, the expected mean motion of the reference stars.A theoretical Galaxy model is defined on an inertial coordinate frame. Proper motions are measured in a reference frame defined by a fundamental catalog. The observed distribution of proper motions in star catalogs can be directly compared with the expected distributions evaluated using IASG to check the accuracy of the adopted reference frame in realizing the inertial coordinate frame in the sky.

Economic performance of migrant entrepreneurs in the high-tech sector: design and application of the GALAXY model

2013 ◽  
pp. 227-260 ◽  
Author(s):  
Mediha Sahin ◽  
Alina Todiras ◽  
Peter Nijkamp ◽  
Enno Masurel
Keyword(s):  
Economic Performance ◽  
High Tech ◽  
High Tech Sector ◽  
The Galaxy ◽  
Galaxy Model ◽  
Migrant Entrepreneurs ◽  
Design And Application

scholarly journals A new dynamically self-consistent version of the Besançon Galaxy model

2018 ◽  
Vol 620 ◽  
pp. A103 ◽  
Author(s):  
O. Bienaymé ◽  
J. Leca ◽  
A. C. Robin
Keyword(s):  
Distribution Functions ◽  
Stellar Kinematics ◽  
Integral Of Motion ◽  
Stellar Component ◽  
Approximate Integral ◽  
Self Consistent ◽  
The Galaxy ◽  
Galaxy Model ◽  
Stellar Orbit ◽  
Self Consistency

Context. Dynamically self-consistent galactic models are necessary for analysing and interpreting star counts, stellar density distributions, and stellar kinematics in order to understand the formation and the evolution of our Galaxy. Aims. We modify and improve the dynamical self-consistency of the Besançon Galaxy model in the case of a stationary and axisymmetric gravitational potential. Methods. Each stellar orbit is modelled by determining a Stäckel approximate integral of motion. Generalised Shu distribution functions (DFs) with three integrals of motion are used to model the stellar distribution functions. Results. This new version of the Besançon model is compared with the previous axisymmetric BGM2014 version and we find that the two versions have similar densities for each stellar component. The dynamically self-consistency is improved and can be tested by recovering the forces and the potential through the Jeans equations applied to each stellar distribution function. Forces are recovered with an accuracy better than one per cent over most of the volume of the Galaxy.

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