A Black Hole Life Preserver
Since no one lives forever, all a life preserver can really do is prolong life for longer than would have
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Since no one lives forever, all a life preserver can really do is prolong life for longer than would have
We previously determined abundances of He, C, N, O, and Ne for a sample of planetary nebulae (PNe) representing a
The Far Ultraviolet Spectroscopic Explorer (FUSE) has surveyed a large sample (> 100) of active galactic nuclei in the low
We have simulated the formation and evolution of large-scale structure in the universe, for 68 different COBE-normalized cosmological models. For
Summary talk given at the International Workshop on Linear Colliders LCWS 99, Sitges (Barcelona), April 28 - May 5, 1999
This paper was withdrawn by the authors.
Registration and management of users in a large scale Grid computing environment presents new challenges that are not well addressed
We study the mechanical and conformational properties of networks of helical polymers with a combination of Monte Carlo simulations based
We present a new evolutionary synthesis (ES) tool specifically developed for the analysis of multi-color data of young star clusters
We propose and evaluate the feasibility of a new strategy to search for planets via microlensing observations. This new strategy
We summarize our recent result for a splitting function for small x evolution which includes resummed small x logarithms deduced
We report on results from a 2003 February INTEGRAL observation of the black hole candidate (BHC) 4U 1630-47 and the
Using media with extremely low group velocities one can create an optical analog of a curved space-time. Leonhardt and Piwnicki
We present results from 3.6 cm observations of the quasar pair 1038+528 A and B, made in 1995 using the
The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable
In this paper, we show that astrophysical accretion disks are dynamically unstable to non-axisymmetric disturbances. This instability is present in
In this paper, we mainly present a new simple, efficient and nondestructive Raman scattering analysis method to study the distribution
Ultraviolet fluorescence (UVF) is introduced as a novel and versatile method for the determination of the contamination of metal impurities
We study the efficient approximability of basic graph and logic problems in the literature when instances are specified hierarchically as
We discovered independently the shell-type supernova remnant G12.82-0.02, recently reported by Brogan et al. (2005), which is coincident with the
We review estimates of the metallicities in elliptical galaxies, with an emphasis on recent results from the ASCA satellite. X-ray
Paper withdrawn by author. New treatment is in preparation.
We summarize the results of an X-ray spectroscopic survey of radio-loud AGNs observed with ASCA, using proprietary and archival data
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