The Massive Accreting Black Hole at the Center of the Milky Way*
Andreas Eckart, R. Genzel, R. Schödel
Abstract
Andreas Eckart, R. Genzel, R. Schödel
Abstract
The Galactic Center is the best established case for a super-massive black hole. Its mass is of the order of 3–4 million solar masses and can be associated with the compact variable radio source Sagittarius A* (SgrA*) and shows powerful flare activity both at X-ray and near-infrared wavelengths. A recent simultaneous detection of such a flare with the VLT and Chandra in both of these spectral bands suggests that they are physically linked and probably originate from the same population of electrons.
OpenAlex reports 3 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The Galactic Center is the best established case for a super-massive black hole. Its mass is of the order of 3–4 million solar masses and can be associated with the compact variable radio source Sagittarius A* (SgrA*) and shows powerful flare activity both at X-ray and near-infrared wavelengths. A recent simultaneous detection of such a flare with the VLT and Chandra in both of these spectral bands suggests that they are physically linked and probably originate from the same population of electrons.
Key concepts: Sagittarius A*, Physics, Galactic Center, Milky Way, Supermassive black hole, Astrophysics, Intermediate-mass black hole, Black hole (networking)