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- Abell 1201 BGC is a massive elliptical galaxyresiding as the brightest cluster galaxy of the galaxy cluster. At a redshift of 0.169, this system is around 2.7 billion light-years from Earth, and offset about 11 kiloparsecs from the X-ray peak of the intracluster gas. With an ellipticity of 0.32±0.02, the stellar distribution is far from spherical. In solar units, the total stellar luminosity is 4×1011 L☉ in SDSS r-band, and 1.6×1012 L☉ in 2MASS K-band. Half the stars orbit within an effective radius of 15 kpc, and their central velocity dispersion is about 285 km s−1 within 5 kpc rising to 360 km s−1 at 20 kpc distance. The BCG also acts as a gravitational lens, bending the light of a more distant background galaxy (at redshift 0.451) into an apparent tangential arc about 6 kpc to one side. This makes the galaxy an important case in investigations of the intrinsic properties of dark matter. Detailed models of the lens mass distribution, starlight and stellar kinematics indicates that the galaxy cluster's dark halo has a shallow inner density gradient and perhaps a soft dark matter core. At face value, this is incompatible with the dark matter cusp predicted by collisionless Cold dark matter theories, and adds to evidence that dark matter experiences additional non-gravitational forces. Years later, a faint smaller counterimage to the arc was discovered at a closer radius. Explaining the position and brightness of this counterimage requires a dark central concentration of unseen mass. Based on lens modelling, it could be a supermassive black hole equivalent to 13 billion suns: 1.3±0.6)×1010 M☉. At the time of measurement, this is one of the most massive black hole candidates (without relying on assumptions about quasar luminosities and efficiencies). This UMBH may be ten times larger than expected from the usual scaling relations between black holes and host galaxies. However, alternative methods of modelling the stellar velocity dispersion maps (accounting for an aggregate constraint on the lens mass) reveals an ambiguity between the UMBH mass and the dark halo profile. In solutions where the UMBH is more massive, the dark matter is more cuspy. In solutions where the UMBH is smaller or absent, the dark matter is more cored. The dark halo's ellipticity and the mass-to-light ratio of stars also enter the ambiguity. Thus, if the standard computational models are robust, then Abell 1201 BCG presents a dilemma and a challenge to either the conventional ideas of black hole growth or the simplest theories about dark matter, or both. (en)
- Abell 1201 BGC est une galaxie elliptique massive résidant en tant que la galaxie la plus brillante de l'amas de galaxies Abell 1201, c'est une galaxie BCG (Brightest Cluster Galaxy). Le terme galaxie BCG signifie que cette galaxie est la plus brillante de l'amas dans laquelle elle se situe, comme dit dans le nom Abell 1201 BCG dans l'amas de galaxie Abell 1201. Cet amas se situe dans la constellation du Lion à 2,7 milliards d'années-lumière de la Terre. (fr)
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- 7190 (xsd:nonNegativeInteger)
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- A picture of A1201 BGC taken by MUSE. (en)
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- R. J. Smith et al, and European Southern Observatory (en)
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- E3 elliptical galaxy, brightest cluster galaxy (en)
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- Abell 1201 BGC est une galaxie elliptique massive résidant en tant que la galaxie la plus brillante de l'amas de galaxies Abell 1201, c'est une galaxie BCG (Brightest Cluster Galaxy). Le terme galaxie BCG signifie que cette galaxie est la plus brillante de l'amas dans laquelle elle se situe, comme dit dans le nom Abell 1201 BCG dans l'amas de galaxie Abell 1201. Cet amas se situe dans la constellation du Lion à 2,7 milliards d'années-lumière de la Terre. (fr)
- Abell 1201 BGC is a massive elliptical galaxyresiding as the brightest cluster galaxy of the galaxy cluster. At a redshift of 0.169, this system is around 2.7 billion light-years from Earth, and offset about 11 kiloparsecs from the X-ray peak of the intracluster gas. With an ellipticity of 0.32±0.02, the stellar distribution is far from spherical. In solar units, the total stellar luminosity is 4×1011 L☉ in SDSS r-band, and 1.6×1012 L☉ in 2MASS K-band. Half the stars orbit within an effective radius of 15 kpc, and their central velocity dispersion is about 285 km s−1 within 5 kpc rising to 360 km s−1 at 20 kpc distance. (en)
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- Abell 1201 BCG (en)
- Abell 1201 BCG (fr)
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- Abell 1201 BCG (en)
- PGC 1430978 (en)
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