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19962026
most citedHigher Charmonia

809 citations · 28.2k across the 927 of their papers we have counts for

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Showing 2005Show all

34 papers · 1 filter

astro-ph2005★ 56 cited

High redshift FRII radio galaxies: X-ray properties of the cores

E. Belsole, D. M. Worrall, M. J. Hardcastle

We present an extensive X-ray spectral analysis of the cores of 19 FRII sources in the redshift range 0.5<z<1.0 which were selected to be matched in isotropic radio power. The samp…

astro-ph2005★ 24 cited

A data-driven Bayesian approach for finding young stellar populations in early-type galaxies from their UV-optical spectra

L. A. Nolan, M. O. Harva, A Kaban +1

We present the results of a novel application of Bayesian modelling techniques, which, although purely data driven, have a physically interpretable result, and will be useful as an…

astro-ph2005★ 2 cited

The XMM-Newton Slew Survey: towards the XMMSL1 catalogue

M. P. Esquej, B. Altieri, D. Bermejo +4

The XMM-Newton satellite is the most sensitive X-ray observatory flown to date due to the great collecting area of its mirrors coupled with the high quantum efficiency of the EPIC…

astro-ph2005★ 15 cited

INTEGRAL high energy behaviour of 4U 1812-12

A. Tarana, A. Bazzano, P. Ubertini +5

The low mass X-ray binary system 4U 1812-12 was monitored with the INTEGRAL observatory in the period 2003-2004 and with BeppoSAX on April 20, 2000. We report here on the spectral…

astro-ph2005

Extended sources in the XMM-Newton slew survey

V. Lazaro, R. Saxton, A. M. Read +4

The low background, good spatial resolution and great sensitivity of the EPIC-pn camera on XMM-Newton give useful limits for the detection of extended sources even during the short…

hep-ph2005★ 9 cited

HADRON05 Summary: Heavy Quark Hadrons and Theory

T. Barnes

This HADRON05 summary covers the topics of (1) mesons containing heavy quarks, and (2) theory. The new material discussed here is taken mainly from plenary presentations. We specif…

astro-ph2005★ 309 cited

Fast neutral outflows in powerful radio galaxies: a major source of feedback in massive galaxies

R. Morganti, C. N. Tadhunter, T. A. Oosterloo

We report the detection of fast (~ 1000 km/s), massive outflows of neutral gas observed -- using the WSRT -- as 21-cm HI absorption against the strong radio continuum of seven radi…

cond-mat.str-el2005

2D Ferromagnetism in the High-Tc Analogue Cs_2AgF_4

S. E. McLain, D. A. Tennant, J. F. C. Turner +5

Although the precise mechanism of high-Tc superconductivity in the layered cuprates remains unknown, it is generally thought that strong 2D Heisenberg antiferromagnetism combined w…

astro-ph2005★ 461 cited

The Secular Evolution of Disk Structural Parameters

Victor P. Debattista, Lucio Mayer, C. Marcella Carollo +3

We present a comprehensive series of -body as well as -body + SPH simulations to study the secular evolution of the structure of disk galaxies. Our simulations are organized…

astro-ph2005★ 14 cited

A further 'degree of freedom' in the rotational evolution of stars

V. Holzwarth, M. Jardine

Observational and theoretical investigations provide evidence for non-uniform spot and magnetic flux distributions on rapidly rotating stars, which have a significant impact on the…

astro-ph2005★ 76 cited

Controlling the collimation and rotation of hydromagnetic disk winds

Ralph E. Pudritz, Conrad Rogers, Rachid Ouyed

(Abriged) We present a comprehensive set of axisymmetric, time-dependent simulations of jets from Keplerian disks whose mass loading as a function of disk radius is systematically…

astro-ph2005★ 60 cited

The kinetic temperature of a molecular cloud at redshift 0.7: Ammonia in the gravitational lens B0218+357

C. Henkel, N. Jethava, A. Kraus +6

Using the Effelsberg 100-m telescope, absorption in the (J,K) = (1,1), (2,2) and (3,3) inversion lines of ammonia (NH_3) was detected at a redshift of z = 0.6847 toward the gravita…

astro-ph2005★ 27 cited

PHASES High Precision Differential Astrometry of delta Equulei

Matthew W. Muterspaugh, Benjamin F. Lane, Maciej Konacki +4

delta Equulei is among the most well-studied nearby binary star systems. Results of its observation have been applied to a wide range of fundamental studies of binary systems and s…

nlin.CD2005★ 22 cited

Chaotic Dynamics of a Free Particle Interacting Linearly with a Harmonic Oscillator

Stephan De Bievre, Paul E. Parris, Alex A. Silvius

We study the closed Hamiltonian dynamics of a free particle moving on a ring, over one section of which it interacts linearly with a single harmonic oscillator. On the basis of num…

astro-ph2005★ 5 cited

A Spitzer/IRAC Survey of the Orion Molecular Clouds

S. T. Megeath, K. M. Flaherty, J. Hora +9

We present initial results from a survey of the Orion A and B molecular clouds made with the InfraRed Array Camera (IRAC) onboard the Spitzer Space Telescope. This survey encompass…

hep-ph2005★ 33 cited

Charmonium production in p pbar annihilation: Estimating cross sections from decay widths

A. Lundborg, T. Barnes, U. Wiedner

The cross sections for the charmonium production processes p pbar -> m Psi, where m is a light meson and Psi is a charmonium state, are of great interest for the planned p-pbar exp…

astro-ph2005★ 37 cited

"PAH" emission bands in selected planetary nebulae: a study of the behaviour with gas phase C/O ratio

Martin Cohen, Michael J. Barlow

Airborne and space-based low-resolution spectroscopy in the 1980s discovered tantalizing quantitative relationships between the gas phase C/O abundance ratio in planetary nebulae (…

astro-ph2005★ 10 cited

FUSE observations of molecular hydrogen on the line of sight towards HD141569A

C. Martin-Zaidi, M. Deleuil, T. Simon +5

We present an analysis of the Far Ultraviolet Spectroscopic Explorer (FUSE) spectrum of HD141569A, a transitional object known to possess a circumstellar disk. We observe two compo…

astro-ph2005★ 5 cited

Can a photometric redshift code reliably determine dust extinction?

T. S. R Babbedge, R. Whitaker, S. Morris

Photometric redshifts can be routinely obtained to accuracies of better than 0.1 in Delta(z)/(1+z). However, the issue of dust extinction is one that has still not been well quanti…

hep-ph2005★ 809 cited

Higher Charmonia

T. Barnes, S. Godfrey, E. S. Swanson

This paper gives results for the spectrum, all allowed E1 radiative partial widths (and some important M1 widths) and all open-charm strong decay amplitudes of all 40 c-cbar states…

cond-mat.mes-hall2005★ 2 cited

Differential Conductance Peak Exchange in Borromean Ring Single Molecule Transistors

Gavin D. Scott, Kelly S. Chichak, Andrea J. Peters +3

While Single Molecule Transistors have been employed in laboratory research for a number of years, there remain many details related to charge transport that have yet to be delinea…

hep-ph2005★ 33 cited

Study of theory and phenomenology of some classes of family symmetry and unification models

G. L. Kane, S. F. King, I. N. R. Peddie +1

We review and compare theoretically and phenomenologically a number of possible family symmetries, which when combined with unification, could be important in explaining quark, lep…

physics.plasm-ph2005★ 3 cited

Dynamic positive column in long-gap barrier discharges

A. Shvydky, V. N. Khudik, V. P. Nagorny +1

A simple analytical model of the barrier discharge in a long gap between opposing plane electrodes is developed. It is shown that the plasma density becomes uniform over large part…

astro-ph2005★ 57 cited

The effect of a finite mass reservoir on the collapse of spherical isothermal clouds and the evolution of protostellar accretion

E. I. Vorobyov, Shantanu Basu

Motivated by recent observations which detect an outer boundary for starless cores, and evidence for time-dependent mass accretion in the Class 0 and Class I protostellar phases, w…