The Filamentary Funnels That Form Stars
The universe is full of fascinating structures, and some of the most striking take shape inside the giant clouds where stars are born. There, streams of gas app...
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How Heavy Can a Neutron Star Get?
The physics of neutron stars are almost too fantastic to believe. Something the weight of two Suns compacted to a sphere the size of a city. Each teaspoon of it...
[2605.31091] Metamorphoses of carbon and oxygen in protoplanetary discs: how chemistry and radial drift transform inner disc C
Abstract page for arXiv paper 2605.31091: Metamorphoses of carbon and oxygen in protoplanetary discs: how chemistry and radial drift transform inner disc C/O ra...
[2605.31132] High-redshift GRB 140304A at z = 5.282 with flaring activity: A multi-wavelength study
Abstract page for arXiv paper 2605.31132: High-redshift GRB 140304A at z = 5.282 with flaring activity: A multi-wavelength study
[2605.31198] Neutron Star Equation of State via Physics Informed Neural Network
Abstract page for arXiv paper 2605.31198: Neutron Star Equation of State via Physics Informed Neural Network
[2605.31290] Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
Abstract page for arXiv paper 2605.31290: Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
![[2605.31301] An Automated Photometric Pipeline for the 80cm Xizang University Telescope](/static/img/curated/desks/afbytes-china.png)
[2605.31301] An Automated Photometric Pipeline for the 80cm Xizang University Telescope
Abstract page for arXiv paper 2605.31301: An Automated Photometric Pipeline for the 80cm Xizang University Telescope
[2605.31335] Gravothermal Collapse: Robust Against Baryonic Feedback
Abstract page for arXiv paper 2605.31335: Gravothermal Collapse: Robust Against Baryonic Feedback
[2605.31362] Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays
Abstract page for arXiv paper 2605.31362: Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays
[2605.31402] Refining the Gaia DR3 Parallax Zero-point: A Hybrid Approach Combining Global Parametric Correction with Local Refinement
Abstract page for arXiv paper 2605.31402: Refining the Gaia DR3 Parallax Zero-point: A Hybrid Approach Combining Global Parametric Correction with Local Refinem...
[2605.31412] MAUVE-MUSE: When Metallicity Follows or Fights Star Formation -- A Mass-Dependent Inversion in Virgo Galaxies
Abstract page for arXiv paper 2605.31412: MAUVE-MUSE: When Metallicity Follows or Fights Star Formation -- A Mass-Dependent Inversion in Virgo Galaxies
[2605.31415] COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $μ$m Since $z=3$
Abstract page for arXiv paper 2605.31415: COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $μ$m Since $z=3$
Scientists Found a Black Hole That Breaks The Rules of Astrophysics
Somewhere in the future, there's a finish line in the marathon to understand supermassive black holes (SMBHs).
'Lost World' of Gravitational Waves Reveals The Origins of Black Holes
Of all the objects in the Universe, few are as perplexing as black holes.
The gold in an ordinary wedding ring was not made on Earth, or even inside an ordinary star, but in the most violent events in the universe, the collisions of dead stars and the flares of magnetised n
The popular version of where gold comes from has become almost a set piece. The metal in a wedding ring was forged in the collision of two neutron stars, drifte...
[2605.28644] Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering
Abstract page for arXiv paper 2605.28644: Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering
[2605.28658] Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks
Abstract page for arXiv paper 2605.28658: Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks
[2605.28662] Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts
Abstract page for arXiv paper 2605.28662: Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts
[2605.28676] Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks
Abstract page for arXiv paper 2605.28676: Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks
[2605.28719] A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$λ$ Trends in Three Gas-Giant Mass Regimes
Abstract page for arXiv paper 2605.28719: A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$λ$ Trends in Three Gas-Giant Mass Regimes
[2605.28731] MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods
Abstract page for arXiv paper 2605.28731: MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding met...
[2605.28755] Hidden worlds: a non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163
Abstract page for arXiv paper 2605.28755: Hidden worlds: a non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163
[2605.28768] The unique ability of the Hubble Space Telescope to characterize young exoplanet environments
Abstract page for arXiv paper 2605.28768: The unique ability of the Hubble Space Telescope to characterize young exoplanet environments
[2605.28771] Evolution of the dusty nova QY Mus from eruption to quiescence
Abstract page for arXiv paper 2605.28771: Evolution of the dusty nova QY Mus from eruption to quiescence
[2605.28777] The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
Abstract page for arXiv paper 2605.28777: The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive st...
[2605.28758] Cluster-centric trends in bar size and pattern speed: the case of Abell 2199
Abstract page for arXiv paper 2605.28758: Cluster-centric trends in bar size and pattern speed: the case of Abell 2199
A New Model Helps Astronomers Study How Merging Black Holes Ring
A new statistical model reveals more details about the ringdown period of merging black holes.