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Summary - X-ray Astronomy Group at ISAS
... forward As Suzaku has shown even ‘small’ improvements can have major science implications ...
The Historical X-ray Transient KY TrA in quiescence
The masses and spins of neutron stars and stellar
systems - Research in Astronomy and Astrophysics
David L. Meier, , 84 (2001); DOI: 10.1126/science.291.5501.84
Launch Tool - Science NetLinks
PS1-10jh: The Disruption of a Main-Sequence Star of Near
Investigating Black Hole Kicks
formation of z 6 quasars from hierarchical
A Universe of Disks
Cosmological Implications of Trace
The first gravitational-wave source from the isolated evolution of two
Roche accretion of stars close to massive black holes
The Formation and Evolution of Massive Black Holes - Ira-Inaf
Can we detect intermediate mass ratio inspirals?
Is there a Supermassive Black Hole at the Center of the Milky Way?
black hole masses and host galaxy evolution of radio
Black Holes in Neutron Stars
Abstract Non-relativistic Quantum Theory fairly accurately describes
Orbiting Light.latex - for blackholeformulas.com
2. Bright AGN phase
Ultraluminous X-ray Sources in Andromeda Galaxy
Document
Binary Black Hole Accretion Flows in Merged Galactic Nuclei
The relation among black holes, their host galaxies and AGN activity
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