ASPEN WINTER 2015 CONFERENCE poster PAPERS
posters can be prepared with any reasonable shape and size, and they will remain on display at the ACP throughout the meeting. On Tuesday there will be a special poster viewing lunch session, with food and drinks provided, immediately following the morning talk session.
Ben Bar-Or and Tal Alexander (Weizmann Institute of Science, Israel): Steady State Relativistic Stellar Dynamics around a Massive Black Hole (poster)
Ben Bar-Or and Tal Alexander (Weizmann Institute of Science, Israel): Relativistic Orbits around a Massive Black Hole – The statistical Mechanics Approach (poster)
Vivienne Baldassare (University of Michigan): Nucleation Fraction in the Field versus Cluster Environment (poster)
Drew
Clausen
(Caltech): Coronal
Emission
Line
Light
Echoes
Following
Tidal
Disruption
Events
Toshihiro Kawaguchi (NAO, Japan): Relics of Galaxy Merging: Observational Predictions for a Wandering Massive Black Hole and Accompanying Star Cluster in the M31 Halo (poster)
Aleksey
Generozov
(Columbia): Circumnuclear
Mediums
and
Accretion
Rates
Quiescent
Supermassive
Black
Holes (poster)
Marion Grould (Observatoire de Paris, France): Relativistic Orbits in the Galactic Center and General Relativity Tests with Gravity
Brunetto Marco Ziosi & Michela Mapelli (INAF): Influence of the Structural Properties of Star Clusters on the Formation and Evolution of Black Hole Binaries
Ryan
OLeary
(JILA): The
Peculiar
Pulsar
Population
of
the
Central
Parsec
Richard
O'Shaughness
(Rochester
Institute
of
Technology): Understanding
and
evolving
precessing
black
hole
binaries (poster)
Laura Shishkovsky (Michigan State University): A Radio Continuum Search for Black Holes in the Milky Way Globular Cluster M10 (poster)
Mario
Spera,
Michela
Mapelli,
Alessandro
Bressan
(INAF,
Italy): The
Mass
Spectrum
of
Compact
Remnants
from
the
PARSEC
Stellar
Evolution
Tracks (poster)
Jong Suk Hong and Hyung Mok (Seoul National University, South Korea): The
Black Hole Binaries in Galactic Nuclei and Gravitational Wave Sources
Long Wang (Peking University, China): NBODY6++GPU Ready for Million-Body Globular Cluster Simulation – Black Hole Evolution (poster)
|
