GRAVITY - Exploring Physics Close to the Galactic Center Black Hole with Infrared Interferometry
APA
Gillessen, S. (2014). GRAVITY - Exploring Physics Close to the Galactic Center Black Hole with Infrared Interferometry. Perimeter Institute. https://pirsa.org/14110091
MLA
Gillessen, Stefan. GRAVITY - Exploring Physics Close to the Galactic Center Black Hole with Infrared Interferometry. Perimeter Institute, Nov. 12, 2014, https://pirsa.org/14110091
BibTex
@misc{ pirsa_PIRSA:14110091, doi = {10.48660/14110091}, url = {https://pirsa.org/14110091}, author = {Gillessen, Stefan}, keywords = {Strong Gravity}, language = {en}, title = {GRAVITY - Exploring Physics Close to the Galactic Center Black Hole with Infrared Interferometry}, publisher = {Perimeter Institute}, year = {2014}, month = {nov}, note = {PIRSA:14110091 see, \url{https://pirsa.org}} }
Max Planck Institute for Physics, Munich (Werner-Heisenberg-Institut)
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Abstract
GRAVITY is a new instrument combining the four 8m ESO Very Large Telescopes in Chile. Other than the BlackHoleCam / EHT with its focus on imaging the shadow of the black hole against the surrounding accretion flow, the goal of GRAVITY is to measure dynamical processes in the immediate vicinity of the black hole, for example the motion of matter close to the last stable orbit and relativistic effects in stellar orbits. Our presentation covers the experimental and astrophysical aspects of this project and highlights the complementarity with the submm interferometry to overcome the degeneracies in modelling the observations.