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相关论文: A Little Red Dot at $\mathbf{z=7.3}$ within a Larg…

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One of the most surprising results of early James Webb Space Telescope (JWST) observations is the discovery of an abundance of red, compact, broad-line objects dubbed "little red dots" (LRDs) at $z>4$. Their spatial density…

We propose an alternative physical interpretation and formation pathway for the recently discovered "little red dots" (LRDs). We model LRDs as super-massive stars (SMSs) surrounded by massive self-gravitating accretion discs (SMDs) that…

星系天体物理 · 物理学 2026-03-04 Lorenz Zwick , Christopher Tiede , Lucio Mayer

We present simulated counterparts of the ``Little Red Dot'' (LRD) galaxies observed with JWST, using the large cosmological hydrodynamic simulation, ASTRID. We create mock observations of the galaxies ($5 \leq z \leq 8$) in ASTRID, and find…

宇宙学与河外天体物理 · 物理学 2026-01-21 Patrick LaChance , Rupert A. C. Croft , Tiziana Di Matteo , Yihao Zhou , Fabio Pacucci , Yueying Ni , Nianyi Chen , Simeon Bird

The Little Red Dots (LRDs) are high-redshift galaxies uncovered by JWST, characterized by small effective radii ($R_{\rm eff} \sim 80-300$ pc), number densities that are intermediate between those of typical galaxies and quasars, and a…

星系天体物理 · 物理学 2025-08-12 Fabio Pacucci , Abraham Loeb

Little Red Dots (LRDs) are a new class of compact extragalactic objects, with a v-shaped optical spectral energy distribution breaking close to the Balmer break wavelength, and broad, typically exponentially-shaped lines. They are believed…

星系天体物理 · 物理学 2025-10-09 G. P. Nikopoulos , D. Watson , A. Sneppen , V. Rusakov , K. E. Heintz , J. Witstok , G. Brammer

Numerical simulations have established that star clusters with densities comparable to the high redshift ($z>6$-$10$) James Webb Space Telescope (JWST) proto globular clusters may build up extremely massive (EMSs; $m_\mathrm{\star}>1000…

星系天体物理 · 物理学 2026-04-28 Antti Rantala

One of the most puzzling discoveries by JWST is the population of high-redshift, red, and compact galaxies dubbed little red dots (LRDs). Based on broad-line diagnostics, these galaxies have been argued to host accreting $10^7-10^8$…

星系天体物理 · 物理学 2025-07-30 Andrea Sacchi , Akos Bogdan

The abundant population of "Little Red Dots" (LRDs)-compact objects with red UV to optical colors and broad Balmer lines at high redshift-is unveiling new insights into the properties of early active galactic nuclei (AGN). Perhaps the most…

Little Red Dots (LRDs) are enigmatic, compact, red galaxies at high redshift, $z\sim 4$-$7$, discovered by the James Webb Space Telescope. Broad emission lines in the absence of X-ray and radio counterparts suggest that they host accreting…

高能天体物理现象 · 物理学 2026-04-29 Riku Kuze , Kunihito Ioka , Kohta Murase , Shigeo S. Kimura , Kohei Inayoshi

JWST has revealed a population of low-luminosity AGN at $z>4$ in compact, red hosts (the "Little Red Dots", or LRDs), which are largely undetected in X-rays. We investigate this phenomenon using GRRMHD simulations of super-Eddington…

高能天体物理现象 · 物理学 2024-11-15 Fabio Pacucci , Ramesh Narayan

Recent James Webb Space Telescope observations have revealed a peculiar class of galaxies at redshifts $z \gtrsim 6$, characterized by extremely high central stellar densities and overmassive central supermassive black holes (SMBHs),…

星系天体物理 · 物理学 2025-06-09 Fazeel Mahmood Khan , Benjamin L. Davis , Andrea Valerio Macciò , Kelly Holley-Bockelmann

Little red dots (LRDs) newly discovered with JWST are active galactic nuclei (AGN) that may represent black hole (BH) growth at the earliest cosmic epochs. These sources show puzzling features unlike typical AGNs, including red optical…

星系天体物理 · 物理学 2026-03-04 Hiroya Umeda , Kohei Inayoshi , Yuichi Harikane , Kohta Murase

The James Webb Space Telescope (JWST) has discovered a new population of objects, the Little Red Dots (LRDs), characterized by V-shaped spectra indicative of strong breaks around the Balmer limit and compact morphology that gave them their…

We investigate the possibility that the recently identified population of high-redshift, obscured quasars - known as "Little Red Dots" (LRDs) - originates from early black hole seed formation driven by ultra-strongly self-interacting dark…

星系天体物理 · 物理学 2026-03-10 M. Grant Roberts , Lila Braff , Aarna Garg , Stefano Profumo , Tesla Jeltema

We present a study of Pseudo-LRD-NOM (Pseudo little red dot with no metal lines), a highly magnified low-mass galaxy behind the lensing cluster Abell 370 at z=5.96. We classify this object as a pseudo-LRD because its red rest-frame optical…

星系天体物理 · 物理学 2026-01-19 Karina I. Caputi , Ryan A. Cooper , Pierluigi Rinaldi , Rafael Navarro-Carrera , Edoardo Iani

The James Webb Space Telescope has detected massive black holes (BHs) with masses of $\sim 10^{6-8}~M_\odot$ within the first billion years of the universe. One of the remarkable findings is the identification of "Little Red Dots" (LRDs), a…

星系天体物理 · 物理学 2025-07-17 Kohei Inayoshi

New populations of red active galactic nuclei (known as ``Little Red Dots'') discovered by JWST exhibit remarkable spectral energy distributions. Leveraging X-ray through far-infrared observations of two of the most luminous known Little…

"Little red dots" (LRDs) represent a new population of astronomical objects uncovered by JWST whose nature remains debated. Although many LRDs are suspected as active galactic nuclei (AGN), they show little variability on days-years…

Little Red Dots (LRDs) are a newly identified class of active galactic nuclei (AGNs) uncovered by JWST deep surveys. Their enigmatic properties challenge the canonical AGN paradigm and have stimulated ideas on early massive black hole (BH)…

星系天体物理 · 物理学 2025-12-04 Kohei Inayoshi , Luis C. Ho

As an unprecedented large population in the early universe, the JWST-discovered little red dots (LRDs) have garnered much attention for formation of massive black holes and galaxies, but their nature remains a mystery. The LRDs appearing as…