Cover - GCNEWS, Vol. 16, October 2003
GCNEWS
A Newsletter for Galactic Center Research
This Volume was edited by Angela Cotera, Sera Markoff & Loránt Sjouwerman
email: gcnews@aoc.nrao.edu

Volume 16, October 2003
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Color composite Image of the Chandra Sgr A* Field
Figure:
Three-color, smoothed image of the Sgr A* field. The red band
is made from photons between 0.5-2.0 keV, the green from 2.0-4.0 keV,
and the blue from 4.0-8.0 keV. The red sources lie in the foregound,
and were not included in the analysis in this paper. Otherwise, the
bulk of the diffuse emission is observed from the Galactic center
between 2-8 keV. The point sources located near the Galactic center are
most prominent in the 4-8 keV band as described
in the invited article in this issue (see Article by Michael Muno).
Click here for a PostScript version of the figure.
Table of Contents
- In the News - Angela Cotera
- "GCNEWS is back!"
- "GC02 Conference Proceedings"
- "In this volume"
- Invited Article: "Can Unresolved Point Sources Produce the Diffuse X-ray Emission from the Galactic Center?", by Michael Muno
- Abstracts of recently submitted papers
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Credits:
- Editors of this Volume: Angela Cotera, Heino Falcke & Sera Markoff
- The GCNEWS Logo
at the top of this page shows a 20cm radio map of the GC (Sgr A) made by Yusef-Zadeh & Morris.
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Heino Falcke.
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National Radio Astronomy Observatory in Socorro NM/USA.
Page currently maintained by
L. O. Sjouwerman.
File last modified on Thursday 09 October 2003 [16:02 MDT].
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\articletitleTable of Contents
\articletitle\seventeenrm In the News
Angela Cotera
\addcontentslinetocsection In the News \it- Angela Cotera
GCNEWS is back!