Nuclear Star Clusters and Black Holes

Nuclear Star Clusters and Black Holes

We summarize the recent results of our survey of the nearest nuclear star clusters. The purpose of the survey is to understand nuclear star cluster formation mechanisms and constrain the presence of black holes using adaptive optics assisted integral field spectroscopy, optical spectroscopy, and HST...

Bibliografski detalji
Glavni autori:	Seth, A, Cappellari, M, Neumayer, N, Caldwell, N, Bastian, N, Olsen, K, Blum, R, Debattista, V, McDermid, R, Puzia, T, Stephens, A
Format:	Conference item
Izdano:	2010

Slični predmeti

THE NGC 404 NUCLEUS: STAR CLUSTER AND POSSIBLE INTERMEDIATE-MASS BLACK HOLE
od: Seth, A, i dr.
Izdano: (2010)

Nearby early-type galactic nuclei at high resolution: Dynamical black hole and nuclear star cluster mass neasurements
od: Nguyen, D, i dr.
Izdano: (2018)

Stellar populations and star formation histories of the nuclear star clusters in six nearby galaxies
od: Kacharov, N, i dr.
Izdano: (2018)

Are Nuclear Star Clusters the Precursors of Massive Black Holes?
od: Nadine Neumayer, i dr.
Izdano: (2012-01-01)

Erratum to “Are Nuclear Star Clusters the Precursors of Massive Black Holes?”
od: Nadine Neumayer, i dr.
Izdano: (2012-01-01)

Resolved nuclear kinematics link the formation and growth of nuclear star clusters with the evolution of their early- and late-type hosts
od: Pinna, F, i dr.
Izdano: (2021)

The nuclear orbital distribution in galaxies as a fossil record of black hole formation from integral-field spectroscopy
od: Cappellari, M, i dr.
Izdano: (2005)

Determination of masses of the central black holes in NGC 524 and 2549 using laser guide star adaptive optics
od: Krajnovic, D, i dr.
Izdano: (2009)

Constraining the role of star cluster mergers in nuclear cluster formation: simulations confront integral-field data
od: Hartmann, M, i dr.
Izdano: (2011)

Two channels of supermassive black hole growth as seen on the galaxies mass-size plane
od: Krajnović, D, i dr.
Izdano: (2017)

Improved dynamical constraints on the masses of the central black holes in nearby low-mass early-type galactic nuclei and the first black hole determination for NGC 205
od: Nguyen, D, i dr.
Izdano: (2019)

Improved dynamical constraints on the mass of the central black hole in NGC 404
od: Nguyen, D, i dr.
Izdano: (2017)

Detection of enhanced central mass-to-light ratios in low-mass early-type galaxies: Evidence for black holes?
od: Pechetti, R, i dr.
Izdano: (2017)

Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters
od: Hartmann, M, i dr.
Izdano: (2010)

Merger rates of intermediate-mass black hole binaries in nuclear star clusters
od: Fragione, G, i dr.
Izdano: (2022)

Weighing black holes using open-loop focus corrections for LGS-AO observations of galaxy nuclei at Gemini Observatory
od: McDermid, R, i dr.
Izdano: (2010)

Weighing black holes using open-loop focus corrections for LGS-AO observations of galaxy nuclei at Gemini Observatory
od: McDermid, R, i dr.
Izdano: (2010)

The structure of nuclear star clusters in nearby late-type spiral galaxies from Hubble Space Telescope wide field camera 3 imaging
od: Carson, DJ, i dr.
Izdano: (2015)

Six new supermassive black hole mass determinations from adaptive-optics assisted SINFONI observations
od: Thater, S, i dr.
Izdano: (2019)

Do Nuclear Star Clusters and Supermassive Black Holes Follow the Same Host-Galaxy Correlations?
od: Peter Erwin, i dr.
Izdano: (2012-01-01)

Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions
od: Das, A, i dr.
Izdano: (2021)

Demographics of Hierarchical Black Hole Mergers in Dense Star Clusters
od: Giacomo Fragione, i dr.
Izdano: (2023-01-01)

Binary Black Hole Mergers and Intermediate-mass Black Holes in Dense Star Clusters with Collisional Runaways
od: Rujuta A. Purohit, i dr.
Izdano: (2024-01-01)

Lower-mass-gap Black Holes in Dense Star Clusters
od: Claire S. Ye, i dr.
Izdano: (2024-01-01)

The black hole in NGC 3379: a comparison of gas and stellar dynamical mass measurements with HST and integral-field data
od: Shapiro, K, i dr.
Izdano: (2006)

Young Star Clusters Dominate the Production of Detached Black Hole–Star Binaries
od: Ugo Niccolò Di Carlo, i dr.
Izdano: (2024-01-01)

Spatial and kinematic segration star cluster merger remnants
od: Cole, D, i dr.
Izdano: (2016)

Anisotropic Star Clusters around Recoiling Supermassive Black Holes
od: Tatsuya Akiba, i dr.
Izdano: (2023-01-01)

Resonant dynamical friction in nuclear star clusters: rapid alignment of an intermediate-mass black hole with a stellar disk
od: Szolgyen, A, i dr.
Izdano: (2021)

BINARY BLACK HOLES IN DENSE STAR CLUSTERS: EXPLORING THE THEORETICAL UNCERTAINTIES
od: Chatterjee, Sourav, i dr.
Izdano: (2017)

Effect of mass-loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters
od: Das, A, i dr.
Izdano: (2021)

MAGICS. III. Seeds Sink Swiftly: Nuclear Star Clusters Dramatically Accelerate Seed Black Hole Mergers
od: Diptajyoti Mukherjee, i dr.
Izdano: (2025-01-01)

Nuclear Physics with Gravitational Waves from Neutron Stars Disrupted by Black Holes
od: Teagan A. Clarke, i dr.
Izdano: (2023-01-01)

The central parsecs of Centaurus A: High Excitation Gas, a Molecular Disk, and the Mass of the Black Hole
od: Neumayer, N, i dr.
Izdano: (2007)

VLT diffraction-limited imaging and spectroscopy in the NIR: Weighing the black hole in Centaurus A with NACO
od: Haring-Neumayer, N, i dr.
Izdano: (2006)

Repeated mergers, mass-gap black holes, and formation of intermediate-mass black holes in dense massive star clusters
od: Fragione, G, i dr.
Izdano: (2022)

Suppressing star formation in quiescent galaxies with supermassive black hole winds
od: Cheung, E, i dr.
Izdano: (2016)

“Blame it on the Black Star”: Black Holes in Culture
od: Mario Rodriguez
Izdano: (2023-12-01)

A low upper-mass limit for the central black hole in the late-type galaxy NGC 4414
od: Thater, S, i dr.
Izdano: (2016)

Clusters of Primordial Black Holes
od: Konstantin M. Belotsky, i dr.
Izdano: (2019-03-01)