2004Progress of Theoretical Physics SupplementRequires access

The Massive Accreting Black Hole at the Center of the Milky Way*

Andreas Eckart, R. Genzel, R. Schödel

Open publisher page 3 citations

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.

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What this paper is about

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.

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Available 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.

Key concepts: Sagittarius A*, Physics, Galactic Center, Milky Way, Supermassive black hole, Astrophysics, Intermediate-mass black hole, Black hole (networking)

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