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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Artemis II – Welcome Home. Podsumowanie misji
› Sławosz Uznański-Wiśniewski uhonorowany tytułem doktora honoris causa Szkoły Głównej Handlowej w Warszawie
› Scanway S.A. i Łukasiewicz – ILOT łączą siły
› Najsłynniejsze zdjęcia Ziemi z kosmosu
› Misje kosmiczne XX wieku: program Energia-Buran
› Relacja z Zimowych Warsztatów Naukowych 2026 w Opolu
› Rekord odległości ludzi od Ziemi. Artemis II wraca do domu
› Spotkaj ekspertkę: Efekty misji IGNIS – kosmiczna opaska zdrowia
› Film poklatkowy (timelapse) w astrofotografii
› Start misji Artemis II – od podstaw
RSS  Najnowsze prace na astro-ph:

› Finite temperature effects on g-modes of inviscid neutron stars
› Sensitivities of Black Hole Images from GRMHD Simulations
› JWST Observations of Starbursts: Dust Processing in the M82 Superwind
› An XMM-Newton Analysis of the Supermassive Black Hole Binary Candidate MCG+11--11--032
› Spectral index evolution of the limb-brightened jet in 3C 84
› A Deep ALMA Survey of the Redshift Distribution of Dusty Star-forming Galaxies
› A sample of short-lived Galactic radio transients from ASKAP VAST
› SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations
› Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy
› Distinct First-to-Second Peak Yield Ratios and Timescales Reveal a Sub-dominant Prompt Channel
› Consistency of the dark matter halo perturbation parameter from morphological and kinematic lopsidedness of galaxies
› The Shocking Origin of the Flat $EE/BB$ Ratio
› A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06
› Beyond the Diffusion Coefficient: Propagators and Memory in Cosmic Ray Transport
› Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0
› Hybrid Simulations of Supersonic Shear Flows: II) Cosmic Ray Viscosity
› JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI
› Introducing $\Delta V_{\star-g}$: a new universal kinematic disturbance parameter
› Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars
› A Forward, Analytic, Differentiable, Geometric (But Inflexible) Lens Model
› An Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
› Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends
› How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
› The role of small-scale environments in the quenching of massive galaxies at $1
› No Country for Old Stars -Spectroscopic confirmation of the first intermediate-age RR Lyrae in the open cluster Trumpler 5
› Reconstructing chemical enrichment pathways in disc galaxies: A phylogenetic approach
› Relativistic Effects on Circumbinary Orbit Stability
› OB runaway stars originating in the Vel OB1 association
› Effective field theory of a single scalar pion field for large scale structure in the Universe
› Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe
› Constraints on Coupled Dark Energy in the DESI Era
› Homogeneous accretion of the Earth in the inner Solar System
› Mapping the emission and spectral properties of the FRI radio galaxy 3C 449 with LOFAR and the VLA
› The exponential growth of infinitesimal perturbations in the long-term evolution of simulated galaxies
› Astrophysical parameters of LS 437 and the nature of X0726-260
› Disk instability model incorporating a variable inner disk radius in SS Cyg and U Gem
› Active moons in our Solar System and beyond -- Io, Europa, Enceladus, Triton, and exomoons
› Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility
› On the possibility of chemically driven convection in red giants. Implications for the He-core flash and mixing above the Red Giant Branch Bump
› Inspecting Cloudy Substellar Atmospheres with JWST MIRI Synthetic Magnitudes from Spitzer Mid-infrared Spectra
› A First Principles Approach to the 100,000-year Problem
› Spatially Resolved Kinematics of SLACS Lens Galaxies. II: Breaking Degeneracies with Lensing and Dynamical Models
› Probing Collapsed Dark Matter Halos with Fast Radio Bursts
› 21 cm Power Spectrum Analysis of North Celestial Pole Observations with the Tianlai Dish Pathfinder Array
› JWST/MIRI Hydrocarbon and Water Absorption in the Wind of a Young Disk: Signatures of Pebble Drift and Carbon Grain Sublimation
› In Situ Interferometric Spatial Mapping Of A Microwave Kinetic Inductance Detector Array
› FRTSearch: Unified Detection and Parameter Inference of Fast Radio Transients using Instance Segmentation
› Detection and analysis of white-light emission in solar flares through light curve diagnostics
› KIC 3868420: A high-amplitude $\delta$ Scuti-$\gamma$ Dor hybrid star crossing the Hertzsprung gap
› Enhancing Ly{\alpha} Emitter Identification in HETDEX with a Convolutional Neural Network
› Accretion-Mode Transition: The Driver Behind Spectral Changes in Changing-Look AGNs
› The $\mu$ Herculis system solved after nearly three centuries
› Multiwavelength Study of Blue Straggler Stars in Tombaugh 2: Evidence for Binary Mass Transfer and Constraints on Cluster Dynamical State
› Interaction-powered Type Ibn Supernovae as a Transient PeVatron Candidate: The Case of SN 2023uqf
› Acoustic instability at shock-wave precursors
› POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean
› Evidence for a bloated massive protostar in IRAS20126+4104
› M1-92: AGB interruption and isotopic ratio paradox. Chemistry and morpho-kinematics from improved shapemol modelling
› Deriving volume density profiles of filaments from observed surface densities
› Primordial Black Holes Formation Beyond the Standard Cosmic QCD Transition
› Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation
› Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow
› Kelvin waves over a differentially rotating spherical shell
› Metal enrichment in the galaxy group IC 1262
› Dark Matter's influence on Evolution of MBHB in Dwarf Galaxies: A Case Study of Leo I dSph
› Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
› The undetectable fraction of core-collapse supernovae in luminous infrared galaxies -- II. GSAOI/GeMS dataset
› Self-Lensing Signals in Binary Systems Containing White Dwarfs with Neutron star or Stellar-mass Black hole Companions
› Illuminating the Local Universe: Large-Scale Structure from ZTF Type Ia Supernovae
› A Search for Hydroacoustic Signals from Bolides
› Constraining Electron-Impact Ionization of O$_2$ Through UV Aurora Observations at Ganymede
› Solar Orbiter observations of solar energetic electron events associated with hard microflares
› Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue
› Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A
› The spectrum of the persistent radio source associated with FRB 20190417A
› A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
› The role of accretion efficiency, natal kicks, and angular momentum transport in the formation of the Gaia black holes
› JWST observations of photodissociation regions. IV. Carbonaceous emission band sub-components in NGC 7023 have distinct spatial distributions
› Hot blue progenitors of stellar-mass black holes
› The $R$-Process Alliance: Actinide Abundances, Variation, and Evolution in Metal-Poor Stars
› Revisiting the angular size-redshift cosmological test with milliarcsecond radio structures in active galactic nuclei
› Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?
› High-energy Processes in the Bubbles of Wolf-Rayet Stars: The case of WR 102
› How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE
› Probing Scalar-Tensor-Induced Gravitational Waves in the nHz Band: $\texttt{NANOGrav}$ and SKA
› Reassessing planetary composition: Evidence of rock-dominated envelopes in Uranus and Neptune
› Obscured at the Core: Evidence for Nuclear Dust in Reddened Type-1 AGN
› A note on Gurzadyan theorem
› Frequency & Radiative Analysis of Random Yagi-UHF/VHF Phased Array
› Amerigo Vespucci and the discovery of the Southern Sky
› Astrophysical Signatures of Einstein-Skyrme Anti-de Sitter Black Holes: Epicyclic Frequencies and QPO Constraints
› RAPRAL v1.0: RAdiation Prediction using RAy tracing and Line-by-line methods for hypersonic air flows
› Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors
› Novel ringdown tests of general relativity with black hole greybody factors
› Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects
› MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU
› Fe-H melting curve below 3 GPa: Implications for hydrogen in the lunar core
› Graviton Production from Inflaton Condensate: Boltzmann vs Bogoliubov
› Dark matter heating of Planet 9, and its observational implications
› Infrared Spectral Gap in a Gluonic Dark Sector as the Origin of the Galactic Acceleration Scale
› Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints
› Jets and spectral states with three-components of accretion flow around a black hole
› Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
› The molecular chemistry of nanoscale organic matter in asteroid Ryugu
› Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascades
› VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
› Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6
› Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias
› Relativistically-strong electromagnetic waves in magnetized plasmas
› The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
› Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses
› The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12
› EFT of Dark Energy with Cosmic Chronometers: Reconstructing Background EFT Functions
› A search for successful and choked jets in nearby broad-lined Type Ic supernovae
› A Shocked Wind Interpretation of an Odd Radio Circle
› The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
› The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-$\chi_{\rm eff}$ correlation
› Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
› Revealing the diversity of Type IIn supernova progenitors through their environments
› POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload
› An Open-Source High-Level Graphical Signal Processing Language with Simulation and HDL Generation
› Self-resonance preheating in deformed attractor models: oscillon formation and evolution
› Measurement prospects for the pair-instability mass cutoff with gravitational waves
› $\texttt{GPUmonty}$: A GPU-accelerated relativistic Monte Carlo radiative transfer code
› Testing models for fully and partially stripped low-mass stars with Gaia: Implications for hot subdwarfs, binary RR Lyrae, and black hole impostors
› Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate
› Comment on: "Third-order corrections to the slow-roll expansion: Calculation and constraints with Planck, ACT, SPT, and BICEP/Keck [2025 PDU 47 101813]"
› New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences
› Formation and disruption of wide binaries in star clusters revealed by N-body simulations
› The multi-age stellar populations of Terzan 5 as revealed by JWST
› AI-Assisted Spectral Decomposition of Euclid Q1 Gravitational Lenses: Extended-Coverage NISP Extraction with Vision-Language Model Quality Control
› DeepDISC-Euclid: Source Classification and Photometric Redshifts in Euclid Deep Field North With a Pixel-Level Deep Learning Approach
› A Statistical-AI Framework for Detecting Transient Flares in SDSS Stripe 82 Quasar Light Curves
› Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune System
› The environmental imprint on molecular layering in the dusty streamer of M512
› Scalar-Induced Electromagnetic Radiation: Comparison with Axion-Like Particles and Implications for Modified Gravity
› Non-degenerate pumping of superconducting resonator parametric amplifier with evidence of phase-sensitive amplification
› BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity
› A Match Made in Heaven: Linking Observables in Inflationary Cosmology
› Properties of the neutron star crust informed by nuclear structure data
› Testing the Dark Universe through the Layzer-Irvine Equation
› Relativistic Maxwell-Bloch Equations with Applications to Astrophysics
› GREA and Dark Energy: A holographic correspondence
› Searches for Post-Merger Gravitational Waves with CoCoA: Sensitivity Projections Across Large Template Banks for Current and Next-Generation Detectors
› Is the Conventional Picture of Coherence Time Complete? Dark Matter Recoherence
› The emergent Big Bang scenario
› Photon Propagation through Magnetar-Hosted Axion Clouds: Time Delays and Polarimetric Constraint

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