Download presentation
Presentation is loading. Please wait.
Published byBeverley Richardson Modified over 9 years ago
1
Max-Planck Institut für Astronomie AGN10 - September 11 th, 2012
2
How do galaxies and BHs coevolve? M BH L Host ** R inf Black holes BLR Host galaxies
3
How do galaxies and BHs coevolve? What are the properties of a galaxy which hosts a QSO? (feedback, AGN triggering,...)
4
L R BLR M BH = G -1 R BLR v BLR 2 R BLR ~ L v BLR = f FWHM CIV – MgII – H
5
0.30.8 Redshift Gain depth through stacking! 340 SDSS images ≈ 1/2 hr 8m class telescope “Population” properties vs. individual objects
6
0.3 0.8 Redshift M BH 5 10 7 2 10 9 15,018 QSOs 446
11
0.3 0.8 Redshift M BH 5 10 7 2 10 9
13
r-z z 0.3<z<0.4
14
r-z z 0.4<z<0.5
15
r-z z 0.5<z<0.6
16
r-z z 0.6<z<0.7
17
r-z z 0.7<z<0.8
18
n sersic R eff [kpc]
25
QSO PSF
26
QSO PSF
27
SFH
28
≡ M BH /M host increases of a factor ~7 from z=0 to z=3 CIV – MgII – H
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.