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8 papers · 2 filters
Monte Carlo Methods for X-ray Dispersive Spectrometers
J. R. Peterson, J. G. Jernigan, S. M. Kahn
We discuss multivariate Monte Carlo methods appropriate for X-ray dispersive spectrometers. Dispersive spectrometers have many advantages for high resolution spectroscopy in the X-…
Deep Searches for Young Pulsars
Fernando Camilo
By 2000 there were only 10 established Galactic pulsar-supernova remnant associations. Two years later there are 16 such associations known. I discuss the work leading to this subs…
X-Ray Spectroscopy and Atomic Data
Ehud Behar, Steven M. Kahn
The Laboratory Astrophysics program employing the Lawrence Livermore National Laboratory (LLNL) Electron Beam Ion Trap (EBIT) has been providing useful atomic data in support of th…
X-ray and Optical Studies of Millisecond Pulsars in 47 Tucanae
C. O. Heinke, J. E. Grindlay, P. D. Edmonds +1
Our Chandra X-ray observation of the globular cluster 47 Tuc clearly detected most of the 16 MSPs with precise radio positions, and indicates probable X-ray emission from the remai…
From Pulsar Spin to Pulsar Wind: The Spectral Connection?
E. V. Gotthelf, C. M. Olbert
We present preliminary results from a systematic spectral study of pulsars and their wind nebulae using the Chandra X-Ray Observatory. The superb spatial resolution of Chandra allo…
The small-scale structure of the Magellanic Stream
S. Stanimirovic, J. M. Dickey, M. Krco +1
We have mapped two regions at the northern tip of the Magellanic Stream in neutral hydrogen 21-cm emission using the Arecibo telescope. The new data are used to study the morpholog…