Reviewing the fundamental instrumental techniques and current observational results, this book unveils the mysteries of the physical processes in the central parsec of our Milky Way: the super-massive black hole embedded in a central stellar cluster as well as the gas and dust in the circumnuclear region.
The observations described cover the entire electromagnetic spectrum from decimeter radio-waves to high energy X-ray and γ-rays, and a comprehensive summary of up-to-date astrophysical interpretations is given.
The emphasis is put on observational techniques, image processing aspects, and a detailed presentation of the most cutting-edge work carried out in the near-infrared wavelength regime. These recent results include both the first orbits of stars around the central black hole and the multiwavelength variability of the central source.
Sample Chapter(s)
Chapter 1: 0bservational Techniques (1,506 KB)
Contents:
- Observational Techniques:The GC Across the Electromagnetic Spectrum
- NIR Imaging Through the Atmosphere
- Speckle Imaging
- Single Telescope Adaptive Optics
- Cleaning and Deconvolution
- Future IR Interferometry
- Observational Results:
- The Discovery of Sagittarius A∗
- Large-Scale Structures at the Galactic Center
- The Circum Nuclear Disk
- The Mini-Spiral
- Radio Filaments
- Near-Infrared Images of the Central Stellar Cluster
- The Radio and Infrared Positional Reference Frames
- Number Density Counts
- Polarization of Filaments and Stars
- Stellar Velocities and Orbital Accelerations
- Spectroscopy
- Star Formation at the Galactic Center?
- Sgr A∗ Across the Electromagnetic Spectrum
- Astrophysical Results:
- The Stellar Velocity Field
- Scenarios for Star Formation at the Galactic Center
- The Central Dark Mass
- Stability of the Enclosed Dark Mass
- Agglomerations of Exotic Particles?
- The Central Stellar Cusp
- Analysis of Stellar Orbits Near the Central Black Hole
- The Central Black Hole
- Comparison to Nuclei of Other Galaxies
- Massive Black Holes at High Redshifts
Readership: Graduate and post-graduate students, researchers, astronomers, and astrophysicists.