'Intermediate mass black holes' presentation slideshows

07.04.27@Ewha

07.04.27@Ewha. Gamma-ray Bursts and Black Holes. Chang-Hwan Lee @. Contents. Motivations. SHB. Short-hard Gamma-ray burst. L-GRB. Long-duration Gamma-ray bursts. Hypernova. Spin of Stellar Mass Black Holes. before BH. before BH formation. at birth. at the time of BH formation.

887 views • 78 slides

07.04.04@KASI

07.04.04@KASI. Spin of Stellar Mass Black Holes: Key to Gamma-ray Bursts & Hypernovae. Chang-Hwan Lee @. Contents. Motivations. GRB. Hypernova. Spin of Stellar Mass Black Holes. before BH. before BH formation. at birth. at the time of BH formation. after BH. after BH formation. GRB.

805 views • 65 slides

Black Holes and Close Binary Star Systems

924 views • 59 slides

The Nuclear Spectroscopic Telescope Array

The Nuclear Spectroscopic Telescope Array. NuSTAR. Varun Bhalerao on behalf of the NuSTAR team. What is NuSTAR?.

689 views • 51 slides

Chapter 22

637 views • 47 slides

From INTEGRAL to SIMBOL-X

448 views • 31 slides

BH Astrophys . Ch4 Intermediate Mass Black Holes

BH Astrophys . Ch4 Intermediate Mass Black Holes. Outline. 1. The definition Possible candidates: 2. ULXs (Ultra-luminous X-ray sources) in star-forming galaxies 3. Globular cluster cores in our Milky Way and Andromeda 4. Possible IMBH near the center of the Milky Way

409 views • 28 slides

Black Holes

Black Holes. The mass of a neutron star cannot exceed about 3 solar masses . If a core remnant is more massive than that, nothing will stop its collapse , and it will become smaller and smaller and denser and denser.

294 views • 28 slides

The Swansong of Stars Orbiting Massive Black Holes

The Swansong of Stars Orbiting Massive Black Holes. Clovis Hopman Weizmann Institute of Science Israel. Advisor : Tal Alexander. Dissipative stellar processes near Massive Black Holes. Tidally powered stars in the Galactic Center Ultraluminous X-ray sources Gravitational Wave Radiation.

344 views • 23 slides

Optical counterparts to Ultraluminous X-ray sources

Optical counterparts to Ultraluminous X-ray sources. Jeanette Gladstone - University of Alberta T. P. Roberts (U of Durham), A. D. Goulding (CfA) T. Cartwright & C. O. Heinke, (U of A), C. Copperwheat & A. J. Levan (U of Warwick), M. R. Goad (U of Leceister).

322 views • 15 slides

Optical counterparts to Ultraluminous X-ray sources

Optical counterparts to Ultraluminous X-ray sources. Jeanette Gladstone - University of Alberta T. P. Roberts (U of Durham), A. D. Goulding (CfA) T. Cartwright & C. O. Heinke, (U of A), C. Copperwheat & A. J. Levan (U of Warwick), M. R. Goad (U of Leceister).

183 views • 15 slides

Status of the Search for Black Hole Ringdowns in LIGO S4 Data

Status of the Search for Black Hole Ringdowns in LIGO S4 Data. Lisa Goggin, Caltech (for the LSC) GWDAW 11 Potsdam, Germany G060616-00-Z. Black Hole Perturbations. If a newly formed black hole exists in a perturbed state, the perturbations will be radiated away as gravitational waves.

234 views • 13 slides

Spectral states of NS and BH systems

137 views • 13 slides

115 views • 1 slides