activity
20022009
most citedFaint Thermonuclear Supernovae from AM Canum Venaticorum Binaries

411 citations · 494 across the 4 of their papers we have counts for

collaborators

11 papers

astro-ph.GA20096 cited

The Galactic Center: A Laboratory for Fundamental Astrophysics and Galactic Nuclei

A. Ghez, M. Morris, J. Lu +24

As the closest example of a galactic nucleus, the Galactic center presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environs. Detailed s…

astro-ph200850 cited

Nonlinear Saturation of g-modes in Proto-Neutron Stars: Quieting the Acoustic Engine

Nevin N. Weinberg, Eliot Quataert

According to Burrows et al.'s acoustic mechanism for core-collapse supernova explosions, the primary, l=1, g-mode in the core of the proto-neutron star is excited to an energy of ~…

astro-ph200727 cited

Carbon Detonation and Shock-Triggered Helium Burning in Neutron Star Superbursts

Nevin N. Weinberg, Lars Bildsten

The strong degeneracy of the 12C ignition layer on an accreting neutron star results in a hydrodynamic thermonuclear runaway, in which the nuclear heating time becomes shorter than…

astro-ph2007411 cited

Faint Thermonuclear Supernovae from AM Canum Venaticorum Binaries

Lars Bildsten, Ken J. Shen, Nevin N. Weinberg +1

Helium that accretes onto a Carbon/Oxygen white dwarf in the double white dwarf AM Canum Venaticorum (AM CVn) binaries undergoes unstable thermonuclear flashes when the orbital per…

astro-ph2005

Astrometric Monitoring of Stellar Orbits at the Galactic Center with a Next Generation Large Telescope

Nevin N. Weinberg, Milos Milosavljevic, Andrea M. Ghez

We show that with a Next Generation Large Telescope one can detect the accelerated motions of ~100 stars orbiting the massive black hole at the Galactic center. The positions and v…

astro-ph2005

Exposing the Nuclear Burning Ashes of Radius Expansion Type I X-ray Bursts

Nevin N. Weinberg, Lars Bildsten, Hendrik Schatz

We solve for the evolution of the vertical extent of the convective region of a neutron star atmosphere during a Type I X-ray burst. The convective region is well-mixed with ashes…