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Related papers: Little Red Dots as Globular Clusters in Formation

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The earliest JWST observations have revealed an unexpected abundance of super-early ($z>10$), massive ($M_*\approx 10^9\, M_\odot$) galaxies at the bright-end ($M_{\rm UV}\approx -21$) of the ultraviolet luminosity function (UV LF). We…

Astrophysics of Galaxies · Physics 2023-05-17 A. Ferrara , A. Pallottini , P. Dayal

Early observations with JWST have led to the discovery of an unexpected large density (stellar mass density $\rho_*\approx 10^{6}\,M_{\odot}\,Mpc^{-3}$) of massive galaxies (stellar masses $M_*\geq 10^{10.5}M_{\odot}$) at extremely high…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-26 N. Menci , M. Castellano , P. Santini , E. Merlin , A. Fontana , F. Shankar

Recent observations by the James Webb Space Telescope (JWST) discovered unexpectedly abundant luminous galaxies at high redshift, posing possibly a severe challenge to popular galaxy formation models. We study early structure formation in a…

Astrophysics of Galaxies · Physics 2024-01-25 Shingo Hirano , Naoki Yoshida

Recent wide-field imaging observations of the X-ray luminous cluster RDCSJ1252.9-2927 at z=1.24 uncovered several galaxy groups that appear to be embedded in filamentary structure extending from the cluster core. We make a spectroscopic…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 M. Tanaka , C. Lidman , R. G. Bower , R. Demarco , A. Finoguenov , T. Kodama , F. Nakata , P. Rosati

The discovery of gravitationally lensed stellar clusters at high redshift with the James Webb Space Telescope (JWST) has revealed extremely compact, massive star-forming systems in galaxies at $z > 6$, providing a new window into early…

Astrophysics of Galaxies · Physics 2026-05-13 Floor van Donkelaar , Lucio Mayer , Pedro R. Capelo , Debora Sijacki , Angela Adamo

Local active galactic nuclei (AGNs) in dwarf galaxies are often considered as analogs for the earliest supermassive black holes, although their connections require more comprehensive examinations. Motivated by finding the local analogs of…

Astrophysics of Galaxies · Physics 2026-05-07 Lulu Bao , Chao-Wei Tsai , Jingwen Wu , Jialai Wang

To investigate the rest-frame optical emission of "Little Red Dots", we model the formation of and evolution of quasi-stars, i.e. stellar envelopes supported by the accretion luminosity onto a central black hole, originating from rapidly…

Solar and Stellar Astrophysics · Physics 2026-03-24 J. Roman-Garza , D. Schaerer , C. Charbonnel , T. Fragos , E. Cenci , R. Marques-Chaves , P. Oesch , M. Xiao

The clustering properties of clusters, galaxies and AGN as a function of redshift are briefly discussed. It appears that extremely red objects at z ~ 1, and objects with J-K > 1.7 and photometric redshifts 2 < z_phot < 4 are highly…

[Abridged] This work concerns very faint (R_lim=28 AB mag; M_(stars, lim) ~ 10^8 Msun), UV-selected sub-L* BX galaxies at z~2.3. Stellar masses, dust content, and dust-corrected SFRs are constrained using broadband SED fitting, giving…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Marcin Sawicki

We present the clump populations detected in 18 lensed galaxies at redshifts 1 to 8.5 within the lensing cluster field SMACS0723. The recent JWST Early Release Observations of this poorly known region of the sky have revealed numerous…

Recent high-resolution observations with the Hubble Space Telescope (HST) reveal that young star clusters of extraordinary luminosity and compactness ("super star clusters") are commonly found in starburst systems. Cluster formation appears…

Astrophysics · Physics 2007-05-23 Luis C. Ho

Luminous Compact Blue Galaxies (LCBGs) are an extreme star-bursting population of galaxies that were far more common at earlier epochs than today. Based on spectroscopic and photometric measurements of LCBGs in massive (M >10^15 M_sun),…

Astrophysics of Galaxies · Physics 2016-01-27 S. M. Crawford , Gregory D. Wirth , M. A. Bershady , S. M. Randriamampandry

We present a new sample of strong gravitational lens systems where both the foreground lenses and background sources are early-type galaxies. Using imaging from HST/ACS and Keck/NIRC2, we model the surface brightness distributions and show…

The largest galaxies acquire their mass early on, when the Universe is still youthful. Cold streams violently feed these young galaxies a vast amount of fresh gas, resulting in very efficient star formation. Using a well resolved…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 J. Devriendt , C. Rimes , C. Pichon , R. Teyssier , D. Le Borgne , D. Aubert , E. Audit , S. Colombi , S Courty , Y. Dubois , S. Prunet , Y. Rasera , A. Slyz , D. Tweed

Low mass stars (< 2-2.5 M_sun) exhibit, at all the stages of their evolution, signatures of processes that require challenging modeling beyond the standard stellar theory. In this paper we focus on their peculiarities while they climb the…

Astrophysics · Physics 2016-08-30 Corinne Charbonnel , Ana Palacios

We have measured the 3.6 micron cluster luminosity function (LF) using a sample of 123 galaxy clusters selected from the 4 degree^2 Spitzer First Look Survey (FLS). The clusters were selected on the basis of their R - 3.6 micron colors…

Astrophysics · Physics 2007-05-23 Adam Muzzin , Gillian Wilson , Mark Lacy

Little red dots (LRDs), a population of active galactic nuclei (AGNs) recently discovered by JWST, show distinctive Balmer-transition features, including prominent Balmer absorption, pronounced Balmer breaks, and large equivalent widths of…

Astrophysics of Galaxies · Physics 2025-12-15 Zu Yan , Kohei Inayoshi , Kejian Chen , Jingsong Guo

The James Webb Space Telescope (JWST) has revealed an unexpected excess of UV-bright galaxies at z>10, unaccounted for by extrapolations from pre-JWST observations and theoretical models. Understanding the physical properties and star…

The formation environment of stars in massive stellar clusters is similar to the environment of stars forming in galaxies at a redshift of 1 - 3, at the peak star formation rate density of the Universe. As massive clusters are still forming…

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