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Testing the connection between the X-ray and submillimetre source populations using Chandra

✍ Scribed by A. C. Fabian; Ian Smail; K. Iwasawa; S. W. Allen; A. W. Blain; C. S. Crawford; S. Ettori; R. J. Ivison; R. M. Johnstone; J.-P. Kneib; R. J. Wilman


Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
152 KB
Volume
315
Category
Article
ISSN
0035-8711

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## Abstract In recent work it was demonstrated that narrow‐line Seyfert 1 galaxies, which possessed spectral complexity in the 2–10 keV band were at the same time X‐ray weak. In this contribution I show how X‐ray weakness can be understood in the context of reflection and light bending picture. In