52 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
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
X-rays, γ-rays and neutrinos from collisionless shocks in supernova wind breakouts
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