Abstract
Under the assumption that a hidden AGN contributes a major part of the bolometric flux of the primeval object IRAS F10214+4724, we argue that sensitive X-ray observations would provide crucial information on the metal enriched gas present in the circumnuclear region.
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© 1996 Kluwer Academic Publishers
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Granato, G.L., Franceschini, A., Danese, L. (1996). IR and X-Rays from IRASF10214+4724: A Hidden AGN?. In: Bremer, M.N., van der Werf, P.P., Röttgering, H.J.A., Carilli, C.L. (eds) Cold Gas at High Redshift. Astrophysics and Space Science Library, vol 206. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1726-2_40
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DOI: https://doi.org/10.1007/978-94-009-1726-2_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7273-1
Online ISBN: 978-94-009-1726-2
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