RT Journal Article
T1 On the excitation of the FeK alpha line in AGNs by the impact of beams of highly relativistic electrons on the disk
A1 Gómez De Castro, Ana Inés
A1 Antonicci, A.
AB The propagation of highly relativistic electron beams in dense matter induces a cascade of secondary particles that spreads in the environment redistributing efficiently the beam energy in the medium. Such a highly relativistic beams are expected to be produced in the magnetic reconnection events associated with the flaring activity of the magnetized accretion disks of the AGNs. This contribution presents a quantitative analysis of the possible role of these beams in the excitation of the Fe K alpha line.
PB Wiley
SN 0004-6337
YR 2006
FD 2006
LK https://hdl.handle.net/20.500.14352/50065
UL https://hdl.handle.net/20.500.14352/50065
NO Gómez De Castro, A. I., & Antonicci, A. «On the Excitation of the Fe K α Line in AGNs by the Impact of Beams of Highly Relativistic Electrons on the Disk». Astronomische Nachrichten, vol. 327, n.o 10, diciembre de 2006, pp. 989-92. DOI.org (Crossref), https://doi.org/10.1002/asna.200610678.
DS Docta Complutense
RD 6 abr 2025