Relativistic redshift of the star S0-2 orbiting the Galactic Center supermassive black hole

T Do, A Hees, A Ghez, GD Martinez, DS Chu, S Jia… - Science, 2019 - science.org
The general theory of relativity predicts that a star passing close to a supermassive black
hole should exhibit a relativistic redshift. In this study, we used observations of the Galactic …

An improved distance and mass estimate for Sgr A* from a multistar orbit analysis

A Boehle, AM Ghez, R Schödel, L Meyer… - The Astrophysical …, 2016 - iopscience.iop.org
We present new, more precise measurements of the mass and distance of our Galaxy's
central supermassive black hole, Sgr A*. These results stem from a new analysis that more …

Testing General Relativity with stellar orbits around the supermassive black hole in our Galactic center

A Hees, T Do, AM Ghez, GD Martinez, S Naoz… - Physical Review Letters, 2017 - APS
We demonstrate that short-period stars orbiting around the supermassive black hole in our
Galactic center can successfully be used to probe the gravitational theory in a strong regime …

The Milky Way's nuclear star cluster: Old, metal-rich, and cuspy-Structure and star formation history from deep imaging

R Schödel, F Nogueras-Lara, E Gallego-Cano… - Astronomy & …, 2020 - aanda.org
Context. The environment of Sagittarius A*(Sgr A*), the central black hole of the Milky Way,
is the only place in the Universe where we can currently study the interaction between a …

PALM-3000: exoplanet adaptive optics for the 5 m Hale telescope

R Dekany, J Roberts, R Burruss… - The Astrophysical …, 2013 - iopscience.iop.org
We describe and report first results from PALM-3000, the second-generation astronomical
adaptive optics (AO) facility for the 5.1 m Hale telescope at Palomar Observatory. PALM …

Properties of the remnant clockwise disk of young stars in the Galactic center

S Yelda, AM Ghez, JR Lu, T Do, L Meyer… - The Astrophysical …, 2014 - iopscience.iop.org
We present new kinematic measurements and modeling of a sample of 116 young stars in
the central parsec of the Galaxy in order to investigate the properties of the young stellar …

Search for a variation of the fine structure constant around the supermassive black hole in our Galactic Center

A Hees, T Do, BM Roberts, AM Ghez, S Nishiyama… - Physical review …, 2020 - APS
Searching for space-time variations of the constants of Nature is a promising way to search
for new physics beyond general relativity and the standard model motivated by unification …

Large scale kinematics and dynamical modelling of the Milky Way nuclear star cluster

A Feldmeier, N Neumayer, A Seth, R Schödel… - Astronomy & …, 2014 - aanda.org
Context. Within the central 10 pc of our Galaxy lies a dense cluster of stars. This nuclear star
cluster forms a distinct component of the Galaxy, and similar nuclear star clusters are found …

The distribution of stars around the Milky Way's central black hole-I. Deep star counts

E Gallego-Cano, R Schödel, H Dong… - Astronomy & …, 2018 - aanda.org
Context. The existence of dynamically relaxed stellar density cusps in dense clusters around
massive black holes is a long-standing prediction of stellar dynamics, but it has so far …

The nuclear cluster of the Milky Way: our primary testbed for the interaction of a dense star cluster with a massive black hole

R Schödel, A Feldmeier, N Neumayer… - … and Quantum Gravity, 2014 - iopscience.iop.org
This article intends to provide a concise overview, from an observational point-of-view, of the
current state of our knowledge of the most relevant properties of the Milky Wayʼs nuclear …