Observations of X-ray Sources with the Chandra X-ray Observatory

Details Observations of X-ray Sources with the Chandra X-ray Observatory Observations of X-ray Sources with the Chandra X-ray Observatory

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..apr.j8004g&link_type=abstract

American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #J8.004

Physics

Scientific paper

The Chandra X-ray Observatory (CXO) offers unprecedented angular resolution and sensitivity compared to previous or currently flying X-ray Missions. Results of a number of observations conducted during the previous six months of operation will be presented. Some of the observations include very long exposures toward the Hubble Deep Field North, the supernova remnants 1987A, RCW103, and N103B, the Orion Nebula, the Galactic Center, M82 and a survey of low luminosity Active Galactic Nuclei. This work is a collaboration between scientists at Penn State University, MIT and Caltech. The support for this endeavor comes from NASA through contract NAS8-38252.

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