Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Pixinsight cz.VI – Łączenie zdjęć monochromatycznych w kolorowy obraz
› Co marsjańskie trzęsienia ziemi mówią o jego historii
› Katalog Caldwella: C75
› Silne dowody na atmosferę na skalistej egzoplanecie
› Przełomowe odkrycie! Pierwsza planeta swobodna odkryta i ,,zważona” przez polskich naukowców
› Rozsiewanie nasion za pomocą satelity – projekt Greenstar
› Katalog Caldwella: C98
› Niebo w styczniu 2026 roku
› Podsumowanie roku 2025 w astronomii i astronautyce
› Katalog Caldwella: C19
RSS  Najnowsze prace na astro-ph:

› Intermediate-mass black hole incubators. Gas accretion onto stellar black hole clusters in galactic central molecular zones
› A survey of molecular clouds in the Galactic center's outflow
› New CDM Crisis Revealed by Multi-Scale Cluster Lensing
› Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
› Quantifying Symmetry: Transformation Information for Planetary Nebulae and Supernova Remnants
› MUSEQuBES: Investigating the Physical and Chemical Properties of Circumgalactic Gas Around Ly$\alpha$ Emitters at $z \approx 3.3$
› FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters
› Relativistic jets from millisecond proto-magnetars
› Dense gas linked to star-forming regions photoionised by embedded gamma-ray bursts
› A persistent bow shock in a diskless magnetised accreting white dwarf
› Sahyadri: A simulation suite for the cosmology dependence of the Cosmic Web
› An eclipsing 8.56 minute orbital period mass-transferring binary
› The GRB Intrinsic Duration Distribution: Progenitor Insights Across Cosmic Time
› On the Jeans criterion for hydrostatic and infalling gas
› Galaxy interactions in void substructures: Morphology and stellar populations of two triplets from CAVITY
› Modeling Cosmogenic 10Be During the Heliosphere's Encounter with an Interstellar Cold Cloud
› Evidence of Feedback Effects in Low-luminosity Active Galactic Nuclei Revealed by JWST Spectroscopy
› The LIRA-Ising Model: Estimating the boundaries of irregularly shaped X-ray sources
› Democratic heliocentric coordinates underestimate the rate of instabilities in long-term integrations of the Solar System
› Investigating quenching in Recently Quenched Elliptical galaxies with HI studies
› Reducing the Dimensions of AGN Lightcurve Manifolds
› Identification of three new ULXs in NGC 4631 and NGC 1097: evidence for stellar-mass black holes
› Stellar Rotation in the First Six Million Years: Rotational Velocities and Radii Estimates of T Tauri Stars in IC 5070 and IC 348
› QED V: Variations in metal loading of galactic winds with element nucleosynthetic origin
› Long Term (250 years) Hydrodynamical Simulation of the Supermassive Black Hole Binary OJ287
› The Secret Lives of Open Clusters: a Multiwavelength Examination of Three Open Clusters
› Cascade Processes of Strong and Weak MHD Turbulence
› Baryon Acoustic Oscillations from the C IV Forest with DESI DR2
› The Contribution of Stars, Dust, Neutral Gas and SMBHs in Galaxies to the Cosmic Baryon Inventory
› Observation of the Forbush decrease on 2024 May 10, using the ALPAQUITA air-shower array at the 70-1000 GV rigidity range
› Unraveling Year-Long Radial Velocity Variations in Red Clump Region -- I: Comprehensive analysis of a K0 Giant star, 2 Draconis
› Diverse Origins of Broad H$\alpha$ Lines in Heavily Obscured AGNs Revealed by Multi-epoch Spectroscopy
› Jupiter-like uniform metal enrichment in a system of multiple giant exoplanets
› Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics
› Constraining the Fraction of LIGO/Virgo/KAGRA Binary Black Hole Merger Events Associated with Active Galactic Nucleus Flares
› A youthful Titan implied by improved impact simulations
› Not so Swift: 20 years of multiwavelength observations of Mrk 421 and Mrk 501
› RotCurves: A PYTHON package for efficient modelling and fitting of galactic rotation curves at high-z
› Evaluating the effectiveness of radio frequency interference removal algorithms for single pulse searches
› Self-consistent dynamical models with a finite extent -- V. Smooth radial truncations and phase-space consistency
› Three Models of the Gravitational Potential of the Milky Way
› Direct detection of hydrogen reveals a new macroscopic crustal water reservoir on early Mars
› Anatomy of Empirical Transit Spectra of Mars based on TGO/NOMAD
› Polychromatic pyramid wavefront sensor with MKID technology for high contrast imaging
› Local Group analogues in a cosmological context -- I. Relating velocity structure to the cosmic web
› A new magnitude--redshift relation based on SNe Ia
› On the estimation of Sulfuric Acid Vapor concentrations below the Venus cloud deck using the Akatsuki Radio Science Experiment
› Thermal-timescale accretion does not always yield critical rotation in mass gainers
› Revisiting the Great Attractor: The Local Group's streamline trajectory, cosmic velocity and dynamical fate
› Radio timing constraints on the orbital orientation and component masses of PSR J1455$-$3330
› Reconstructing Gamma Ray Burst Energy Relations with Observational H(z) data in Neural Network Framework
› Substellar population of the young massive cluster RCW 36 in Vela
› On the Interstellar Extinction Curve toward HD 93222, A Sightline with an Exceedingly Narrow 2175 Angstrom Extinction Bump
› Dust Properties of the Interstellar Object 3I/ATLAS Revealed by Optical and Near-Infrared Polarimetry
› Primordial Gravitational Waves from Scalar Backreaction in Axion-SU(2) Inflation
› Rare Near-Opposition Alignment of 3I/ATLAS on 22 January, 2026
› MUSE-ALMA Haloes XIII. Molecular gas in $z \sim 0.5$ HI-selected galaxies
› Blind Deconvolution in Astronomy: How Does a Standalone U-Net Perform?
› One-Loop Tensor Power Spectrum from a Non-Minimally Coupled Spectator Field during Inflation
› Stellar masses of optically dark galaxies: uncertainty introduced by the attenuation law and star-formation histories
› Evolution and afterglow emission of gamma-ray burst jets from binary neutron star mergers
› First direct electron temperature measurement in [O II] zone in I Zw 18
› Evidence of sloshing-driven mini-halo formation in the cool-core cluster RXCJ1558.3-1410
› A precessing jet from an active galactic nucleus drives gas outflow from a disk galaxy
› The drastic impact of Eddington-limit induced mass ejections on massive star populations
› Probing Dark Matter annihilation in the Galactic Centre with TRIDENT
› Ghost-free non-local $F(R)$ Gravity Compatible with ACT
› The Scalar Mach-Sciama Theory of Gravitation
› Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
› Charting the Flavour Structure of Dark Matter
› General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly
› The Topological Origin of Bohm Resistivity in Magnetic Reconnection
› Chiral three-nucleon forces for the new local position-space two-nucleon potential in $\textit{ab initio}$ many-body calculations
› Velocity-Space Signatures of Energy Transfer for Ion-Acoustic Instabilities
› Rotation of the Globular Cluster Population of the Dark Matter Deficient Galaxy NGC 1052-DF4: Implication for the Total Mass
› Revisiting The Cosmological Time Dilation of Distant Quasars: Influence of Source Properties and Evolution
› Power Suppression and Lensing Anomaly -- A phenomenological investigation
› Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii
› A Model of UV-Blue Absorbance in Bulk Liquid of Venusian Cloud Aerosols Is Consistent with Efficient Organic Absorbers at High Concentrations
› Abundant Population of Broad H$\alpha$ Emitters in the GOODS-N Field Revealed by CONGRESS, FRESCO, and JADES
› Many body effects in the line radiative transfer equation
› The Dichotomy in the Nuclear and Host Galaxy Properties of High-redshift Quasars
› Fast Low Energy Reconstruction using Convolutional Neural Networks
› Identifying lopsidedness in spiral galaxies using a Deep Convolutional Neural Network
› Chasing Serendipity: Tackling Transient Sources with Neutrino Telescopes
› A planet-host ratio relation to synthesize microlensing and transiting exoplanet demography from Roman
› Constraints from CMB lensing tomography with projected bispectra
› The impact of kilonova seed photons on GRB VHE emission
› A $\tau-$DM relation for FRB hosts?
› SN 2024hpj: A perspective on SN 2009ip-like events
› 1.8 per cent measurement of $H_0$ from Cepheids alone
› Bias in the tensor-to-scalar ratio from self-interacting dark radiation
› JADES: the chemical enrichment pattern of distant galaxies -- $\alpha$ enhancement, silicon depletion, and iron enhancement
› Searching for Dark Structures: A Comparison of Weak-lensing Convergence Maps and Lensing-weighted Galaxy Density Maps
› Signatures of dark subhalos in dwarf spheroidal galaxies: I. Fluctuations in surface density
› iPTF16geu through the lens of thermonuclear explosion models
› JCMT detection of HCN emission from 3I/ATLAS at 2.1 AU
› A Comoving Framework for Planet Migration
› Coherence of Supermassive Black Hole Binary Demographics with the nHz Stochastic Gravitational Wave Background
› The THESAN-ZOOM project: The Hidden Neighbours of OI Absorbers during Reionization
› Impact of Neutrino Flavor Conversions on Neutron Star Merger Dynamics, Ejecta, Nucleosynthesis, and Multi-Messenger Signals
› XRISM mock observations of simulated AGN jets in the core of a galaxy cluster
› Luminosity-Dependent Assembly Bias of Central Galaxies from Weak Lensing and Clustering
› The Spiral Pattern Speed in the Milky Way Galaxy
› X-rays Emission: a novel tool to detect Extensive Air Showers
› PHANGS-JWST: the largest extragalactic molecular cloud catalog traced by polycyclic aromatic hydrocarbon emission
› A new estimate of the zero-point shift of the Gaia DR3 parallaxes obtained from a comparison with VLBI measurements of masers and radio stars
› J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $
› Optimizing the potential of KM3NeT in detecting core-collapse supernovae
› Spectuner-D1: Spectral Line Fitting of Interstellar Molecules Using Deep Reinforcement Learning
› Variable X-ray Emission of the Planet Hosting T Tauri Star CI Tau
› The SPace-based InterFerometer Feasibility (SPIFF) Project: Enabling Future High-Resolution Astronomy Across the EM Spectrum
› The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
› A secondary orbiter under collisions with an accretion disk
› Rotational Kinematics in the Globular Cluster System of M31: Insights from Bayesian Inference
› A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements
› Multi-wavelength properties of changing-state active galactic nuclei: I. the evolution of soft excess and X-ray continuum
› Angular correlation and deformed Hellings-Downs curve from spin-2 ultralight dark matter
› Evidence for strong isovector nuclear spin-orbit interaction
› Scalar perturbations on the normal and self-accelerating branch of a DGP brane and $\sigma_8$
› Extreme mass ratio inspirals in dark matter halos: dynamics and distinguishability of halo models
› Could a Primordial Black Hole Explosion Explain the extremely high-energy KM3NeT neutrino Event?
› Magnetic field dynamics in presence of Hall conductivity and thermo-diffusion
› Asymptotics of spherical dynamos exhibiting a small-scale MAC balance
› Hydrodynamic models of reheating
› Investigating Production of TeV-scale Muons in Extensive Air Shower at 2400 Meters Underground
› Conserved Quantities in Expanding G\"odel Cosmology

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