Zobrazeno 1 - 10
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pro vyhledávání: '"K. A. Pounds"'
Autor:
K. A. Pounds
Publikováno v:
International Astronomical Union Colloquium. 123:111-118
JET-X is one of the main payload elements in the Soviet Spectrum-X Gamma mission scheduled for launch in 1993. It consists of two Wolter I X-ray telescopes feeding cooled arrays of CCD’s. The combination of good angular resolution and long exposure
Autor:
K. A. Pounds
Publikováno v:
Exploring the Universe.
Publikováno v:
AIP Conference Proceedings.
The evidence for cold matter in AGN, based on X‐ray observations, is discussed. The Fe Kα line equivalent width and reflection hump provide constraints on the geometry and optical depth of such material, but some uncertainties still remain. The sc
Publikováno v:
Physics of Active Galactic Nuclei ISBN: 9783642775680
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a93612acf2bc0554fbf3f2c7da7a8d9
https://doi.org/10.1007/978-3-642-77566-6_4
https://doi.org/10.1007/978-3-642-77566-6_4
Autor:
K. A. Pounds
Publikováno v:
Nature. 374:491-491
Publikováno v:
Space Science Reviews. 48:367-371
Autor:
K A Pounds
Publikováno v:
Transactions of the International Astronomical Union. 19:616-625
The period leading up to the last IAU General Assembly was dominated in X-ray Astronomy by the results from the Einstein Observatory. This first application of a large, satellite-borne, high resolution X-ray telescope to the study of cosmic sources h
Autor:
K. A. Pounds, Andrew C. Fabian
Publikováno v:
Annals of the New York Academy of Sciences. 336:496-519
Surveys of the extragalactic X-ray sky based on data obtained from the Uhuru and Ariel V satellites are considered. The X-ray luminosity function of clusters is discussed the total density of X-ray clusters is found to approach that of all Abell clus
Autor:
K. A. Pounds, T. J. Turner
Publikováno v:
Symposium - International Astronomical Union. 134:155-160
Results are presented from EXOSAT observations of Seyfert type active galactic nuclei (AGN). The sample chosen for study are 48 hard X-ray selected Seyfert type AGN, including all 30 of the emission line AGN in the Piccinotti sample. Combining EXOSAT