Boaz Katz
www.weizmann.ac.il
0000-0003-0584-2920
Weizmann Institute of Science
53 papers found
Refreshing results…
Luminosity function suggests up to 100 white dwarfs within 20 pc may be hiding in multiple systems
Warm Jupiters Need Close “friends” for High-Eccentricity Migration—a Stringent Upper Limit on the Perturber's Separation
AMS-02 Results Support the Secondary Origin of Cosmic Ray Positrons
HEAD-ON COLLISIONS OF WHITE DWARFS IN TRIPLE SYSTEMS COULD EXPLAIN TYPE Ia SUPERNOVAE
The energy production rate density of cosmic rays in the local universe is $∼10^{44-45}\rm erg~Mpc^{-3}~yr^{-1}$ at all particle energies
Non-Relativistic Radiation Mediated Shock Breakouts. Iii. Spectral Properties of Supernova Shock Breakout
An exact integral relation between the Ni56 mass and the bolometric light curve of a type Ia supernova
Exploring a “flow” of Highly Eccentric Binaries Withkepler
Directly Imaging Tidally Powered Migrating Jupiters
The rate of WD-WD head-on collisions may be as high as the SNe Ia rate
Q in Other Solar Systems
Physical Basis for a Constant Lag Time
PANCHROMATIC OBSERVATIONS OF SN 2011dh POINT TO a COMPACT PROGENITOR STAR
Super-Eccentric Migrating Jupiters
Non-Relativistic Radiation Mediated Shock Breakouts. Ii. Bolometric Properties of Supernova Shock Breakout
Radius and magnetic field from synchrotron self-absorbed radio and inverse-Compton X-ray observations of supernovae
Non-Relativistic Radiation-Mediated Shock Breakouts. I. Exact Bolometric Planar Breakout Solutions
Long-Term Cycling of Kozai-Lidov Cycles: Extreme Eccentricities and Inclinations Excited by a Distant Eccentric Perturber
Long-Wavelength Unstable Modes in the Far Upstream of Relativistic Collisionless Shocks
Exponential growth of eccentricity in secular theory
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