output
20022015
most citedNear linear time algorithm to detect community structures in large-scale networks

3.6k citations

Showing 2002 · astro-phShow all

7 papers · 2 filters

astro-ph2002

Some recent developments in gamma-ray burst afterglow and prompt emission models

Bing Zhang, Peter Meszaros, Junfeng Wang

Extensive observational campaigns of afterglow hunting have greatly enriched our understanding of the gamma-ray burst (GRB) phenomenon. Efforts have been made recently to explore s…

astro-ph2002

Feeding the active nucleus of NGC 1097

Thaisa Storchi-Bergmann, Rodrigo Nemmen da Silva, Michael Eracleous

We discuss the signatures of an evolving accretion disk around the nucleus of NGC 1097, based on observations of its double-peaked H-alpha emission-line profile which cover a time…

astro-ph2002

X-ray emission from the most luminous z>4 Palomar Digital Sky Survey Quasars: the Chandra view

C. Vignali, W. N. Brandt, D. P. Schneider +2

We present the results obtained from exploratory Chandra observations of nine high-redshift (z=4.09-4.51) quasars, selected from among the optically brightest Palomar Digital Sky S…

astro-ph2002

Radio pulsar death

Bing Zhang

Pulsar radio emission is believed to be originated from the electron-positron pairs streaming out from the polar cap region. Pair formation, an essential condition for pulsar radio…

astro-ph2002

Pulsar Wind Nebulae and Particle Acceleration in the Pulsar Magnetosphere

S. Shibata, M. Tomatsuri, M. Shimanuki +3

This paper deals with the Crab Nebula problem to suggest that particle acceleration takes place not only at the inner shock but also over a larger region in the nebula with disorde…

astro-ph2002

X-rays from star-forming regions: New objects, new physics, new visions

T. Montmerle, N. Grosso, E. D. Feigelson +1

Star-forming regions have been the targets of X-ray observations since the dawn of satellite X-ray astronomy. The increase in sensitivity and/or spatial resolution offered by XMM-N…