Galaxies with much higher-than-normal luminosities host supermassive black holes (BHs) with masses up to billions of solar masses in their nuclei. The immediate environment around these BHs typically includes an accretion disk of material that gradually falls toward the BH, clouds of hot gas, and a torus of dust and gas that partially obscures the nucleus when the galaxy is edge-on. Relativistic energetic jets of rapid, highly collimated outflows emerge in opposite directions from the poles of the BH. This compact energetic region is called active galactic nucleus (AGN). Depending on how the AGN is tilted towards us, the host galaxy is classified as a type II Seyfert radio galaxy (when viewed edge-on), a type I Seyfert radio galaxy, and a quasar (when the AGN is not obscured by the torus) and a blazar (when the AGN has a jet pointed toward the Earth).
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| ABOUT THE SELLER |
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| SELLER-USER-NAME | Salvatore Orlando |
| 3D Model formats | FBX, OBJ, BLENDER, TEXTURES, Materials |
| 3D Model details | VR / AR / Low-poly, Textures, Materials, UV Mapping, Scale transformations |
| Triangles | 2.3M |
| Vertices | 1.1M |
| Category | Nature & Plants, Science & Technology |
| Tags | accretion-disk, astronomy, astrophysics, black_hole, blackhole, galaxy, high-energy, milkyway, physics, sky, stars, universe |
