activity
19962026
most citedHigher Charmonia

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

collaborators
Showing 2003 · astro-phShow all

25 papers · 2 filters

astro-ph2003★ 25 cited

Atomic lines in infrared spectra for ultracool dwarfs

Yu. Lyubchik, H. R. A. Jones, Ya. V. Pavlenko +3

We provide a set of atomic lines which are suitable for the description of ultracool dwarf spectra from 10000 to 25000 Å. This atomic linelist was made using both synthetic spectra…

astro-ph2003★ 55 cited

The Size of the Longest Filaments in the Universe

Somnath Bharadwaj, Suketu Bhavsar, Jatush V. Sheth

We analyze the filamentarity in the Las Campanas redshift survey (LCRS) and determine the length scale at which filaments are statistically significant. The largest length-scale at…

astro-ph2003★ 23 cited

XMM-Newton observations of two X-ray bright galaxy groups - pushing out to r_500

Jesper Rasmussen, Trevor J. Ponman

We report on the results of XMM-Newton observations of the z=0.18 galaxy group WARPJ0943.7+1644 and the nearby poor cluster WARPJ0943.5+1640 at z=0.256. Tracing the X-ray gas out t…

astro-ph2003

Spectropolarimetry of Compton-thin Seyfert 2s

S. L. Lumsden, D. M. Alexander, J. H. Hough

We present new spectropolarimetry of a sample of nearby Compton-thin Seyfert 2 galaxies (ie those with N_H<10^23 cm^-2). We show that the detection rate of scattered broad Halpha i…

astro-ph2003★ 45 cited

Time Structure of Muonic Showers

L. Cazon, R. A. Vazquez, A. A. Watson +1

An analytical description of the time structure of the pulses induced by muons in air showers at ground level is deduced assuming the production distance distribution for the muons…

astro-ph2003★ 90 cited

XMM-Newton observation of Kepler's supernova remnant

G. Cassam-Chenai, A. Decourchelle, J. Ballet +3

We present the first results coming from the observation of Kepler's supernova remnant obtained with the EPIC instruments on board the XMM-Newton satellite. We focus on the images…

astro-ph2003★ 29 cited

Mid- to Far-Infrared spectroscopy of Sharpless 171

Y. Okada, T. Onaka, H. Shibai +1

We have collected one-dimensional raster-scan observations of the active star-forming region Sharpless 171 (S171), a typical HII region-molecular cloud complex, with the three spec…

astro-ph2003

Radio Cores of Bipolar Nebulae: Search for Collimated Winds

Ting-Hui Lee, Jeremy Lim, Sun Kwok

We present results of our search for collimated ionized winds in bipolar nebulae using the Very Large Array (VLA) and the Australia Telescope Compact Array (ATCA). Our search is mo…

astro-ph2003★ 42 cited

From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs

B. Vollmer, T. Beckert, W. J. Duschl

We compare three different models of clumpy gas disk and show that the Circumnuclear Disk (CND) in the Galactic Center and a putative, geometrically thick, obscuring torus are best…

astro-ph2003★ 35 cited

Arakelian 564: An XMM-Newton view

C. Vignali, W. N. Brandt, Th. Boller +2

We report on two XMM-Newton observations of the bright narrow-line Seyfert 1 galaxy Ark 564 taken one year apart (2000 June and 2001 June). The 0.6-10 keV continuum is well describ…

astro-ph2003★ 24 cited

The orbital period of the dipping, bursting, globular cluster X-ray source XB 1746-371 from Rossi X-ray Timing Explorer observations

M. Balucinska-Church, M. J. Church, A. P. Smale

We present results from two long observations of XB 1746-371 by the Rossi X-ray Timing Explorer (RXTE) in 2002 January and May, lasting 4 and 5 days respectively. Dips are observed…

astro-ph2003★ 108 cited

Exploring the complex X-ray spectrum of NGC 4051

K. A. Pounds, J. N. Reeves, A. R. King +1

Archival XMM-Newton data on the nearby Seyfert galaxy NGC 4051, taken in relatively high and low flux states, offer a unique opportunity to explore the complexity of its X-ray spec…

astro-ph2003★ 1 cited

Testing the locality of transport in self-gravitating accretion discs

Giuseppe Lodato, W. K. M. Rice

In this paper we examine the issue of characterizing the transport associated with gravitational instabilities in relatively cold discs, discussing in particular under which condit…

astro-ph2003★ 48 cited

Radio Loud AGN in the Context of the Eigenvector 1 Parameter Space

J. W. Sulentic, S. Zamfir, P. Marziani +3

We consider the properties of radio-loud (RL) AGN in the context of the Eigenvector 1 (E1) parameter space. RL sources show a restricted E1 parameter space occupation relative to t…

astro-ph2003★ 114 cited

Triggered massive-star formation at the border of the HII region Sh 104

L. Deharveng, B. Lefloch, A. Zavagno +4

We present millimetre-line imaging of the Galactic HII region Sh 104. We show that it is surrounded by a ring of molecular gas and dust. Four large molecular condensations are regu…

astro-ph2003★ 29 cited

Meissner Effect and Vortex Dynamics in Quark Stars -- A Model for Soft Gamma-Ray Repeaters

R. Ouyed, O. Elgaroy, H. Dahle +1

We present a new model for soft gamma-ray repeaters based on a quark star born with temperatures above the critical value (T_c) for the onset of the colour-flavor locked supercondu…

astro-ph2003★ 216 cited

XMM-Newton observation of the brightest X-ray flare detected so far from SgrA*

D. Porquet, P. Predehl, B. Aschenbach +5

We report the high S/N observation on October 3, 2002 with XMM-Newton of the brightest X-ray flare detected so far from SgrA* with a duration shorter than one hour (~ 2.7 ks). The…

astro-ph2003★ 61 cited

XMM-Newton and the Pleiades -- I: Bright coronal sources and the X-ray emission from intermediate-type stars

K. R. Briggs, J. P. Pye

We perform X-ray spectral and timing analyses of solar-like (spectral types F5--K8) and intermediate-type (B4--F4) Pleiads observed in a 40-ks XMM-Newton EPIC exposure. All 8 solar…

astro-ph2003★ 17 cited

The Narrow Line Region of Ark 564

Marcella Contini, Alberto Rodriguez-Ardila, Sueli Viegas

The continuum and emission-line spectrum of the narrow-line Seyfert 1 galaxy Ark 564 is used to investigate, for the first time, the physical conditions and structure of its narrow…

astro-ph2003★ 14 cited

Detection of type-2 quasars in the radio galaxies B3 0731+438 and 3C 257

P. M. Derry, P. T. O'Brien, J. N. Reeves +3

We present XMM-Newton observations and spectral fitting of two highly redshift, [OIII]-luminous, narrow-line radio galaxies, B3 0731+438 and 3C 257. Their X-ray continua are well f…

astro-ph2003★ 69 cited

Numerical 3D constraints on convective eddy time-correlations : consequences for stochastic excitation of solar p modes

R. Samadi, A. Nordlund, R. F. Stein +2

A 3D simulation of the upper part of the solar convective zone is used to obtain information on the frequency component, chi_k, of the correlation product of the turbulent velocity…

astro-ph2003

Zeeman tomography of magnetic white dwarfs: General method and application to EF Eridani

F. Euchner, K. Beuermann, K. Reinsch +3

We have developed a new method to derive the magnetic field distribution on the surfaces of rotating magnetic white dwarfs from phase-resolved flux and circular polarization spectr…

astro-ph2003★ 21 cited

Decline of the space density of quasars between z=2 and z=4

M. Vigotti, R. Carballo, C. R. Benn +5

We define a new complete sample of 13 optically-luminous radio quasars M_AB(1450 Angstrom) < -26.9 mag and log P_1.4 GHz(W/Hz) > 25.7 with redshift 3.8 < z < 4.5, obtained by cross…

astro-ph2003★ 74 cited

Numerical constraints on the model of stochastic excitation of solar-type oscillations

R. Samadi, A. Nordlund, R. F. Stein +2

Analyses of a 3D simulation of the upper layers of a solar convective envelope provide constraints on the physical quantities which enter the theoretical formulation of a stochasti…