Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
Secular evolution and the formation of pseudobulges in disk galaxies
▪ Abstract The Universe is in transition. At early times, galactic evolution was dominated by
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
The apache point observatory galactic evolution experiment (APOGEE)
SR Majewski, RP Schiavon… - The Astronomical …, 2017 - iopscience.iop.org
Abstract The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the
programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic …
programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic …
Nuclear star clusters
We review the current knowledge about nuclear star clusters (NSCs), the spectacularly
dense and massive assemblies of stars found at the centers of most galaxies. Recent …
dense and massive assemblies of stars found at the centers of most galaxies. Recent …
Rapid and bright stellar-mass binary black hole mergers in active galactic nuclei
Abstract The Laser Interferometer Gravitational-wave Observatory (LIGO) found direct
evidence for double black hole binaries emitting gravitational waves. Galactic nuclei are …
evidence for double black hole binaries emitting gravitational waves. Galactic nuclei are …
Assisted inspirals of stellar mass black holes embedded in AGN discs: solving the 'final au problem'
We explore the evolution of stellar mass black hole binaries (BHBs) which are formed in the
self-gravitating discs of active galactic nuclei (AGN). Hardening due to three-body scattering …
self-gravitating discs of active galactic nuclei (AGN). Hardening due to three-body scattering …
[HTML][HTML] The universe at faint magnitudes. I-Models for the galaxy and the predicted star counts
JN Bahcall, RM Soneira - … Series, vol. 44, Sept. 1980, p. 73-110 …, 1980 - adsabs.harvard.edu
The universe at faint magnitudes. I - Models for the galaxy and the predicted st ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …
is now deprecated. It will be completely retired in October 2019. This page will automatically …
The cosmic evolution of binary black holes in young, globular, and nuclear star clusters: rates, masses, spins, and mixing fractions
The growing population of binary black holes (BBHs) observed by gravitational wave (GW)
detectors is a potential Rosetta stone for understanding their formation channels. Here, we …
detectors is a potential Rosetta stone for understanding their formation channels. Here, we …
Unveiling the gravitational universe at μ-Hz frequencies
We propose a space-based interferometer surveying the gravitational wave (GW) sky in the
milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in …
milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in …
Dynamical friction in a gaseous medium
EC Ostriker - The Astrophysical Journal, 1999 - iopscience.iop.org
Using time-dependent linear perturbation theory, we evaluate the dynamical friction force on
a massive perturber M $\mathstrut {_ {p}} $ traveling at velocity $\mathstrut {{\bmi V}} …
a massive perturber M $\mathstrut {_ {p}} $ traveling at velocity $\mathstrut {{\bmi V}} …