BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Talks.cam//talks.cam.ac.uk//
X-WR-CALNAME:Talks.cam
BEGIN:VEVENT
SUMMARY:When the spectral lines in the Seyfert Galaxy NGC 5548 went on hol
 iday - Gary Ferland (U Kentucky)
DTSTART:20190628T103000Z
DTEND:20190628T113000Z
UID:TALK124657@talks.cam.ac.uk
CONTACT:Martin Haehnelt
DESCRIPTION:The emission-line regions in Active Galactic Nuclei (AGN) have
 \ndeveloped the reputation as being complicated with slow progress since\n
 the first models by Bahcall & Kozlovsky in 1969.   Despite this\, they\nar
 e necessary probes of the inner regions  of AGN and a primary\nindicator o
 f the black hole mass.  When the recent HST STORM campaign was poised to p
 roduce the largest and best set of observations of NGC 5548\, the lines de
 cided to go on holiday rather than participate in yet another study. I wil
 l talk about what happened\, and now a disk\nwind can produce it.  This wi
 nd is a likely source of the non-disk\nemission that has been noted by man
 y studies.\n
LOCATION:Kavli Large Meeting Room\, Kavli Building
END:VEVENT
END:VCALENDAR