Galaxy formation and evolution

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Star Formation in Viscous Galaxy Disks

(2000)

Authors:

Adrianne Slyz, Julien Devriendt, Andreas Burkert, Kevin Prendergast, Joseph Silk
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The European Large Area ISO Survey — I. Goals, definition and observations

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 316:4 (2000) 749-767

Authors:

Seb Oliver, Michael Rowan-Robinson, DM Alexander, O Almaini, M Balcells, AC Baker, X Barcons, M Barden, I Bellas-Velidis, F Cabrera-Guerra, R Carballo, CJ Cesarsky, P Ciliegi, DL Clements, H Crockett, L Danese, A Dapergolas, B Drolias, N Eaton, A Efstathiou, E Egami, D Elbaz, D Fadda, M Fox, A Franceschini, R Genzel, P Goldschmidt, M Graham, JI Gonzalez-Serrano, EA Gonzalez-Solares, GL Granato, C Gruppioni, U Herbstmeier, P Héraudeau, M Joshi, E Kontizas, M Kontizas, JK Kotilainen, D Kunze, F La Franca, C Lari, A Lawrence, D Lemke, MJD Linden-Vørnle, RG Mann, I Márquez, J Masegosa, K Mattila, RG McMahon, G Miley, V Missoulis, B Mobasher, T Morel, H Nørgaard-Nielsen, A Omont, P Papadopoulos, I Perez-Fournon, J-L Puget, D Rigopoulou, B Rocca-Volmerange, S Serjeant, L Silva, T Sumner, C Surace, P Vaisanen, PP van der Werf, A Verma, L Vigroux, M Villar-Martin, CJ Willott
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A relationship between nuclear black hole mass and galaxy velocity dispersion

Astrophysical Journal 539:1 PART 2 (2000) L13-L16

Authors:

K Gebhardt, R Bender, G Bower, A Dressler, SM Faber, AV Filippenko, R Green, C Grillmair, LC Ho, J Kormendy, TR Lauer, J Magorrian, J Pinkney, D Richstone, S Tremaine

Abstract:

We describe a correlation between the mass Mbh of a galaxy's central black hole and the luminosity-weighted line-of-sight velocity dispersion σe within the half-light radius. The result is based on a sample of 26 galaxies, including 13 galaxies with new determinations of black hole masses from Hubble Space Telescope measurements of stellar kinematics. The best-fit correlation is Mbh = 1.2(±0.2) × 108 M⊙(σe/200 km s-1)3.75 (±0.3)over almost 3 orders of magnitude in Mbh; the scatter in Mbh at fixed σe is only 0.30 dex, and most of this is due to observational errors. The Mbh-σe relation is of interest not only for its strong predictive power but also because it implies that central black hole mass is constrained by and closely related to properties of the host galaxy's bulge.
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The European Large Area ISO Survey III: 90micron extragalactic source counts

(2000)

Authors:

A Efstathiou, S Oliver, M Rowan-Robinson, C Surace, T Sumner, P Heraudeau, MJD Linden-Vornle, D Rigopoulou, S Serjeant, RG Mann, CJ Cesarsky, L Danese, A Franceschini, R Genzel, A Lawrence, D Lemke, RG McMahon, G Miley, J-L Puget, B Rocca-Volmerange
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Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics

(2000)

Authors:

Karl Gebhardt, John Kormendy, Luis Ho, Ralf Bender, Gary Bower, Alan Dressler, SM Faber, Alexei Filippenko, Richard Green, Carl Grillmair, Tod Lauer, John Magorrian, Jason Pinkney, Douglas Richstone, Scott Tremaine
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