Showing 2000 · astro-phShow all

97 papers · 2 filters

astro-ph2000★ 34 cited

3EG J2016+3657: Confirming an EGRET Blazar Behind the Galactic Plane

J. P. Halpern, M. Eracleous, R. Mukherjee +1

We recently identified the blazar-like radio source G74.87+1.22 (B2013+370) as the counterpart of the high-energy gamma-ray source 3EG J2016+3657 in the Galactic plane. However, si…

astro-ph2000★ 232 cited

Colors of 2625 Quasars at 0<z<5 Measured in the Sloan Digital Sky Survey Photometric System

Gordon T. Richards, Xiaohui Fan, Donald P. Schneider +3

We present an empirical investigation of the colors of quasars in the Sloan Digital Sky Survey (SDSS) photometric system. The sample studied includes 2625 quasars with SDSS photome…

astro-ph2000★ 115 cited

The Quiescent X-Ray Spectrum of the Neutron Star in Cen X-4 Observed with Chandra/ACIS-S

Robert E. Rutledge, Lars Bildsten, Edward F. Brown +2

We report on spectral and intensity variability analysis from a Chandra/ACIS-S observation of the transient, type-I X-ray bursting low-mass X-ray binary Cen X-4. The quiescent X-ra…

astro-ph2000★ 59 cited

ASCA Discovery of Diffuse 6.4 keV Emission Near the Sgr C Complex: A New X-ray Reflection Nebula

H. Murakami, K. Koyama, M. Tsujimoto +2

We present an ASCA discovery of diffuse hard X-ray emission from the Sgr C complex with its peak in the vicinity of the molecular cloud core. The X-ray spectrum is characterized by…

astro-ph2000★ 51 cited

High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data V. Hobby-Eberly Telescope Observations

Donald P. Schneider, Xiaohui Fan, Michael A. Strauss +5

We report the discovery of 27 quasars with redshifts between 3.58 and 4.49. The objects were identified as high-redshift candidates based on their colors in Sloan Digital Sky Surve…

astro-ph2000★ 827 cited

Further Evidence for Cosmological Evolution of the Fine Structure Constant

J. K. Webb, M. T. Murphy, V. V. Flambaum +5

We describe the results of a search for time variability of the fine structure constant, alpha, using absorption systems in the spectra of distant quasars. Three large optical data…

astro-ph2000★ 128 cited

Possible evidence for a variable fine structure constant from QSO absorption lines: systematic errors

M. T. Murphy, J. K. Webb, V. V. Flambaum +2

Comparison of quasar absorption spectra with laboratory spectra allow us to probe possible variations in the fundamental constants over cosmological time-scales. In a companion pap…

astro-ph2000★ 356 cited

Possible evidence for a variable fine structure constant from QSO absorption lines: motivations, analysis and results

M. T. Murphy, J. K. Webb, V. V. Flambaum +5

An experimental search for variation in the fundamental coupling constants is strongly motivated by modern high-energy physics theories. Comparison of quasar absorption line spectr…

astro-ph2000★ 660 cited

The Luminosity Function of Galaxies in SDSS Commissioning Data

SDSS Collaboration, M. R. Blanton

During commissioning observations, the Sloan Digital Sky Survey (SDSS) has produced one of the largest existing galaxy redshift samples selected from CCD images. Using 11,275 galax…

astro-ph2000★ 57 cited

PMN J0525-3343: soft X-ray spectral flattening in a blazar at z=4.4

A. C. Fabian, A. Celotti, K. Iwasawa +5

We report optical, radio and X-ray observations of a new distant blazar, PMN J0525-3343, at a redshift of 4.4. The X-ray spectrum measured from ASCA and BeppoSAX flattens below a f…

astro-ph2000★ 39 cited

Off-Beam Gamma-Ray Pulsars and Unidentified EGRET Sources in the Gould Belt

Alice K. Harding, Bing Zhang

We investigate whether gamma-ray pulsars viewed at a large angle to the neutron star magnetic pole could contribute to the new population of galactic unidentified EGRET sources ass…

astro-ph2000★ 63 cited

Models of Cuspy Triaxial Galaxies

Kelly Holley-Bockelmann, J. Christopher Mihos, Steinn Sigurdsson +1

We construct numerical models of mildly triaxial elliptical galaxies with central density cusps. Using a technique we call ``adiabatic squeezing'', we begin with a spherical gamma=…

astro-ph2000★ 250 cited

Observation of X-ray lines from a Gamma-Ray Burst (GRB991216): Evidence of Moving Ejecta from the Progenitor

L. Piro, G. Garmire, M. Garcia +18

We report on the discovery of two emission features observed in the X-ray spectrum of the afterglow of the gamma-ray burst (GRB) of 16 Dec. 1999 by the Chandra X-Ray Observatory. T…

astro-ph2000★ 27 cited

H-alpha Imaging with HST+NICMOS of An Elusive Damped Ly-alpha Cloud at z=0.6

Nicolas Bouche, James D. Lowenthal, Jane C. Charlton +3

Despite previous intensive ground-based imaging and spectroscopic campaigns and wide-band HST imaging of the z=0.927 QSO 3C336 field, the galaxy that hosts the damped Ly-alpha syst…

astro-ph2000★ 63 cited

Electron-Positron Pair Cascades and Precursors in Gamma-Ray Bursts

P. Meszaros, E. Ramirez-Ruiz, M. J. Rees

Gamma-ray burst sources with a high luminosity can produce electron-positron pair cascades in their environment as a result of back-scattering of a seed fraction of their original…

astro-ph2000★ 741 cited

Gamma-ray Burst Afterglow with Continuous Energy Injection: Signature of a Highly-Magnetized Millisecond Pulsar

Bing Zhang, Peter Meszaros

We investigate the consequences of a continuously injecting central engine on the gamma-ray burst afterglow emission, focusing more specifically on a highly-magnetized millisecond…

astro-ph2000★ 38 cited

BeppoSAX observations of Narrow-Line Seyfert 1 galaxies: II. Ionized iron features in Arakelian 564

A. Comastri, G. M. Stirpe, C. Vignali +8

The BeppoSAX observations of the bright Narrow-Line Seyfert 1 galaxy Ark 564 are presented along with a high quality optical spectrum taken at the 1.5m telescope at La Silla. The 0…

astro-ph2000★ 90 cited

High-resolution X-ray spectroscopy of the Seyfert 2 galaxy Circinus with Chandra

R. M. Sambruna, H. Netzer, S. Kaspi +5

Results from a 60 ks Chandra HETGS observation of the nearby Seyfert 2 Circinus are presented. The spectrum shows a wealth of emission lines at both soft and hard X-rays, including…

astro-ph2000★ 44 cited

X-ray imaging of the Seyfert 2 galaxy Circinus with Chandra

R. M. Sambruna, W. N. Brandt, G. Chartas +5

We present results from the zeroth-order imaging of a Chandra HETGS observation of the nearby Seyfert 2 galaxy Circinus. Twelve X-ray sources were detected in the ACIS-S image of t…

astro-ph2000★ 44 cited

An XMM-Newton detection of the z=5.80 X-ray weak quasar SDSSp J104433.04-012502.2

W. N. Brandt, M. Guainazzi, S. Kaspi +5

We report on an XMM-Newton observation of the most distant known quasar, SDSSp J104433.04-012502.2, at z=5.80. We have detected this quasar with high significance in the rest-frame…

astro-ph2000★ 109 cited

Iron K-alpha Emission from a Decaying Magnetar Model of Gamma-Ray Bursts

M. J. Rees, P. Meszaros

The recent report of X-ray Fe features in the afterglow of the gamma-ray burst GRB 991216 may provide important clues for identifying the nature of its progenitor and constraining…

astro-ph2000★ 36 cited

Nature and Nurture: a model for soft gamma-ray repeaters

Bing Zhang, R. X. Xu, G. J. Qiao

During supernova explosions, strange stars with almost bare quark surfaces may be formed. Under certain conditions, these stars could be rapidly spun down by the torque exerted by…

astro-ph2000★ 91 cited

On the Origin of Intrinsic Narrow Absorption Lines in z<1 QSOs

Rajib Ganguly, Nicholas A. Bond, Jane C. Charlton +3

We present a statistical analysis of the associated, high ionization narrow absorption line (NAL) systems in a sample of 59 QSOs defined from the HST QSO Absorption Line Key Projec…

astro-ph2000

The Assembly and Evolution of Spiral Disks

Matthew Bershady, David Andersen

We explore how the growth rate of spiral disks can be measured via analyses of the scatter in the Tully-Fisher (TF) relation of local and intermediate redshift galaxies. As an init…