Little red dots (LRDs) are a class of small, red-tinted galaxies discovered by the James Webb Space Telescope.[1][2][3] Their discovery was published in March 2024, and they are currently poorly understood.[4] They appear to have existed between 0.6 and 1.6 billion years after the Big Bang, from 13.2 to 12.2 billion years ago.[1]
However, LRDs also exhibit properties that are difficult to explain within the AGN scenario. For example, they have a flat infrared spectrum[6] and lack x-ray detection.[7][8] LRDs also show very weak time variability, often seen in AGN observation.[9]
Several models have been proposed to explain the observed properties of LRDs.[10][11][12] The shape of the ultraviolet spectrum can be explained by the scattered AGN light[10][11] or by the gray dust extinction law.[12]
The gas in LRDs spins extremely fast, at around 3,000 km/h, when the typical gas flow is around 300 km/h.[1] Some scientists argue that the gas is accelerated to these extreme speeds by spinning, supermassive black holes; it has also been argued that LRDs are extremely compact to spin at their speeds.[1] Most are also small, usually around 2% of the radius of the Milky Way.[3]
Likely local analogues of LRDs were discovered in a sample of Green Pea Galaxies (GP). These are broad-line AGN hosting Green Peas (BLGP) with V-shaped rest-frame UV-to-optical SEDs. Seven such V-shaped BLGPs were identified. These V-shaped BLGPs host over-massive black holes.[13]
^Kokubo, Mitsuru; Harikane, Yuichi (2024). "Challenging the AGN scenario for JWST/NIRSpec broad Hα emitters/Little Red Dots in light of non-detection of NIRCam photometric variability and X-ray". arXiv:2407.04777 [astro-ph.GA].
^ abLabbe, Ivo; Greene, Jenny E.; Bezanson, Rachel; Fujimoto, Seiji; Furtak, Lukas J.; Goulding, Andy D.; Matthee, Jorryt; Naidu, Rohan P.; Oesch, Pascal A.; Atek, Hakim; Brammer, Gabriel; Chemerynska, Iryna; Coe, Dan; Cutler, Sam E.; Dayal, Pratika (2023). "UNCOVER: Candidate Red Active Galactic Nuclei at 3 < z < 7 with JWST and ALMA". arXiv:2306.07320 [astro-ph.GA].
^ abLi, Zhengrong; Inayoshi, Kohei; Chen, Kejian; Ichikawa, Kohei; Ho, Luis C. (2024). "Little Red Dots: Rapidly Growing Black Holes Reddened by Extended Dusty Flows". arXiv:2407.10760 [astro-ph.GA].
^Lin, Ruqiu; Zheng, Zhen-Ya; Jiang, Chunyan; Yuan, Fang-Ting; Ho, Luis C.; Wang, Junxian; Jiang, Linhua; Rhoads, James E.; Malhotra, Sangeeta (2024-12-11). "Discovery of Local Analogs to JWST's Little Red Dots". arXiv:2412.08396 [astro-ph].