69 citations · 166 across the 7 of their papers we have counts for
7 papers
A dust-free hierarchically nested supermassive-star model for James Webb Space Telescope Little Red Dots
Pau Amaro Seoane
Observations by the James Webb Space Telescope reveal a population of high-redshift objects, the little red dots. These sources exhibit optical reddening alongside blue ultraviolet…
Monte-Carlo Stellar Dynamics near Massive Black Holes: Two-dimensional Fokker-Planck solutions of multiple mass components
Fupeng Zhang, Pau Amaro Seoane
In this study we present a novel Monte-Carlo code, referred to as GNC, which enables the investigation of dynamical relaxation in clusters comprising multiple mass components in th…
Transient stellar collisions as multimessenger probes: Non-thermal-, gravitational wave emission and the cosmic ladder argument
Pau Amaro Seoane
In dense stellar clusters like galactic nuclei and globular clusters stellar densities are so high that stars might physically collide with each other. In galactic nuclei the energ…
The young stars in the Galactic Center
Sebastiano von Fellenberg, Stefan Gillessen, Julia Stadler +11
We present a large spectroscopic survey of the Galactic Center using the SINFONI IFU at the VLT. Combining observations of the last two decades we compile s…
Excitation of gravitational wave modes by a center-of-mass velocity of the source
Alejandro Torres-Orjuela, Xian Chen, Pau Amaro Seoane
Most gravitational wave (GW) sources are moving relative to us. This motion is often closely related to the environment of the source and can thus provide crucial information about…
Curvature conditions for spatial isotropy
Kostas Tzanavaris, Pau Amaro Seoane
In the context of mathematical cosmology, the study of necessary and sufficient conditions for a semi-Riemannian manifold to be a (generalised) Robertson-Walker space-time is impor…
Merging stellar and intermediate-mass black holes in dense clusters: implications for LIGO, LISA and the next generation of gravitational wave detectors
Manuel Arca-Sedda, Pau Amaro-Seoane, Xian Chen
We study the formation of intermediate-mass ratio inspirals (IMRIs) triggered by the interactions between two stellar black holes (BHs) and an intermediate-mass BH (IMBH) inhabitin…