activity
19942026
most citedCoevolution (Or Not) of Supermassive Black Holes and Host Galaxies

4.2k citations · 53.7k across the 547 of their papers we have counts for

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Showing 2006 · astro-phShow all

9 papers · 2 filters

astro-ph2006★ 233 cited

The Centers of Early-Type Galaxies with HST. VI. Bimodal Central Surface Brightness Profiles

Tod R. Lauer, Karl Gebhardt, S. M. Faber +9

We combine the results from several HST investigations of the central structure of early-type galaxies to generate a large sample of parameterized surface photometry. The studies i…

astro-ph2006★ 32 cited

Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. III. Optical Variability and X-ray/UV/Optical Correlations

Louis-Benoit Desroches, Alexei V. Filippenko, Shai Kaspi +11

We present optical observations of the low-luminosity Seyfert 1 nucleus of NGC 4395, as part of a multiwavelength reverberation-mapping program. Observations were carried out over…

astro-ph2006★ 413 cited

The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes

Tod R. Lauer, S. M. Faber, Douglas Richstone +11

Black hole masses predicted from the Mbh-sigma relationship conflict with those predicted from the Mbh-L relationship for the most luminous galaxies, such as brightest cluster gala…

astro-ph2006★ 209 cited

HST/STIS Spectra of Nuclear Star Clusters in Spiral Galaxies: Dependence of Age and Mass On Hubble Type

Joern Rossa, Roeland P. van der Marel, Torsten Boeker +5

(Abridged) We study the nuclear star clusters in spiral galaxies of various Hubble types using spectra obtained with STIS on-board HST. We observed the nuclear clusters in 40 galax…

astro-ph2006★ 81 cited

Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. I. Method outline

Marc S. Seigar, James S. Bullock, Aaron J. Barth +1

We investigate the use of spiral arm pitch angles as a probe of disk galaxy mass profiles. We confirm our previous result that spiral arm pitch angles (P) are well-correlated with…

astro-ph2006★ 12 cited

Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC 4395. II. X-ray and Ultraviolet Continuum Variability

Paul M. O'Neill, Shai Kaspi, Ari Laor +7

We report on two Chandra observations, and a simultaneous Hubble Space Telescope ultraviolet observation, of the dwarf Seyfert 1 galaxy NGC 4395. Each Chandra observation had a dur…

astro-ph2006★ 57 cited

Contribution of Stellar Tidal Disruptions to the X-Ray Luminosity Function of Active Galaxies

Milos Milosavljevic, David Merritt, Luis C. Ho

The luminosity function of active galactic nuclei has been measured down to luminosities ~10^{42} erg/s in the soft and hard X-rays. Some fraction of this activity is associated wi…

astro-ph2006★ 109 cited

Hubble Space Telescope H-Band Imaging Survey of Massive Gas-Rich Mergers

S. Veilleux, D. -C. Kim, C. Y. Peng +6

We report the results from a deep HST NICMOS H-band imaging survey of a carefully selected sample of 33 luminous, late-stage galactic mergers at z < 0.3. Signs of a recent galactic…

astro-ph2006★ 59 cited

A Radio Census of Nuclear Activity in Nearby Galaxies

M. E. Filho, P. D. Barthel, L. C. Ho

In order to determine the incidence of black hole accretion-driven nuclear activity in nearby galaxies, as manifested by their radio emission, we have carried out a high-resolution…