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

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RSS  Najnowsze prace na astro-ph:

› High Resolution VLA Radio Observations of the Boomerang Pulsar Wind Nebula
› X-Shooting ULLYSES: Massive stars at low metallicity XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds
› ALMA Central Molecular Zone Exploration Survey (ACES) II: 3mm continuum images
› The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6
› Dynamical friction on binary stars in dark matter dominated environments
› Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole Activity
› Cloaking Cosmic Light
› The origin of isolated millisecond pulsars in globular clusters
› Galactic Center Gamma-Ray Excess from a Generic Triaxial Halo
› The First Systematic Survey of Stellar Halos in High-Inclination Galaxies Reveals Unusually Quiescent Merger Histories of Nearby Galaxies
› ALMA Central molecular zone Exploration Survey (ACES) VI: ALMA Large Program Reveals a Highly Filamentary Central Molecular Zone
› Willman 1 Revisited: The Kinematics, Chemistry, and Orbital Properties of a Potentially-Disrupting Dwarf Galaxy
› ALMA Central molecular zone Exploration Survey (ACES) III: Molecular line data reduction and HNCO and HCO$^{+}$ data
› Neural Bayesian updates to populations with growing gravitational-wave catalogs
› Planet formation at the inner edge of the dead zone -- I: the interplay between accretion outbursts and dust growth
› Compute System Organization for High Frequency High Order Wavefront Sensing and Control
› Evidence for Sympathetic Flaring in TESS Data
› BASS LVI. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances
› Inspectorch: Efficient rare event exploration in solar observations
› Quasars behind the disk of M31 galaxy
› ALMA Central Molecular Zone Exploration Survey (ACES) I: Overview
› An automated activity classification tool for optical galaxy spectra
› Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO
› Cosmological Constraints on Neutrino Masses in Quintessential Inflation
› First Observation of CO$_2$ Emission and foreground absorption Toward the Galactic Center with JWST
› A Census Before Rubin of Asteroid Families in the Main Belt
› Glance: A Comprehensive Framework for Galactic Archaeology
› Spatially-resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA2
› Constraining the Sub-Galactic Relationship Between Star Formation and the Hot Interstellar Medium in NGC 4254
› Stellar flare study of nearby young moving group members with TESS Data
› Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
› IR-Safe and IR-Resummed Bispectra Before and After Reconstruction in Unified Lagrangian Perturbation Theory
› Chandra X-ray Observations of Quasars with Velocity-Offset Broad Lines: Assessing the Binary Supermassive Black Hole Hypothesis
› ALMA Central Molecular Zone Exploration Survey (ACES)-IV. Data of the two intermediate-width spectral windows
› Detectability of Satellite Planes in Mock Observations of Isolated L* Galaxies
› Evolution of Spatial Complexity in Flare Ribbon Substructure and Its Relationship to Magnetic Reconnection Dynamics
› Introduction to Strong Alfv\'enic MHD Turbulence
› Machine-learning cosmological parameters by eROSITA data
› Formation of dusty clumps in the torus of active galactic nuclei
› Search for Light-Mass Fractionally Charged Particles in Space with DAMPE Experiment
› ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH?
› AT 2024wpp: the most luminous fast-evolving optical transient linked to the merger explosion of a black-hole binary
› Capture and Stability of Resonant Planet Pairs in Turbulent Disk
› Rotation of a Solar Jet Driven by Plasma Flow along Helical Magnetic Fields in an Active Region
› Constraining the onset height of coronal mass ejection driven shocks using near-Sun observations in visible and radio wavelengths
› 70 years of spectroscopy of the photosphere and the solar chromosphere at the Pic du Midi Observatory (1956-2026)
› PLATOSpec's first results: Three new transiting warm Jupiters from the WINE survey TIC 147027702, TIC 245076932 and TIC 87422071
› Infall onto the Protoplanetary Disk during the Gravitational Collapse of a Molecular Cloud
› Formation of first star clusters under the supersonic gas flow -- III. Environmental trends and halo-to-halo scatter in the Pop III IMF
› Multiple protostellar outflows from a single protostar with a misaligned disk
› F10.7 Index Prediction: A Multiscale Decomposition Strategy with Wavelet Transform for Performance Optimization
› Galaxy evolution in the cosmic web: the relative impact of nodes and filaments in the EAGLE simulation
› Bypassing the Lyth Bound with Entangled Gravitons: Primordial Signatures and Late-Time Noise
› Evidence of a non-equipartition energy regime in 1803+784 Core-shift and Faraday rotation measurements from simultaneous multi-frequency polarimetric VGOS observations
› Long-term optical variability of high-mass X-ray binaries. III. Polarimetry
› SN 2024abvb: a Type Ibn/Icn supernova with evidence of helium and an extreme offset from its host galaxy
› A multi-wavelength study of nearby starburst galaxy M 82
› Cylindrical cosmological simulations with StePS
› Photosynthetic exergy I. Thermodynamic limits for habitable-zone planets
› Infrared spectropolarimetry of a C-class solar flare footpoint plasma -- I. Spectral features and forward modelling
› Characteristics of natural remanence records in fine-grained particles returned from asteroid Ryugu
› Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources
› Stellar structure, magnetism and the variational principle
› Revisiting the Geminga halo at GeV energies with Fermi-LAT data
› A Salpeter IMF and an NFW halo: Disentangling the dark and stellar mass through precise lens modelling of a double-source-plane system reinforces the canonical model of elliptical galaxies
› The Magnetic Filling in MAD Simulations and its Impact on the Jet in M87
› XRISM Discovery of Multiple Ionized Fe-K Emission and Absorption Components in Centaurus A
› Gaia Data Release 4: Modelling of drift-scan related effects in Gaia's point spread function
› Constraints on CMBR flux due to high-z dust emission
› Relativistic Dissipative Magnetohydrodynamics from the Boltzmann equation for 2-particle species gas
› Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare
› Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies
› Black hole-Neutron star distinction based on long-term MAXI and Swift study of 42 low mass X-ray binaries
› Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections
› Molecular bipolar outflow in SN 1987A supports the jittering-jets explosion mechanism
› HINORA II: Testing the Existence of the Council of Giants in {\Lambda}CDM simulations
› A Catalog of 486 Barium Stars Identified in GALAH DR4
› The hybrid Nova Vul 2024 (=V615 Vul)
› Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys
› The no-hair theorems at work in the tidal disruption event AT2020afhd
› MHD Simulations of Strongly Magnetized HII Region Evolution: Evidence for Ionized Gas Filamentation
› Experimental and computational studies of the hydrogenation of carbon disulfide (CS2) on ice analogues
› RAMSES-MCR: A consistent multi-group treatment of cosmic rays physics in momentum-space with the RAMSES code
› Revisiting CPL with sign-switching density: to cross or not to cross the NECB
› Scattering, Migration, Re-circularization and Relaxation to Build Out Galaxy Disks with Exponential Profiles
› The JWST Resolved Stellar Populations Early Release Science Program. IX. The RR Lyrae Population in WLM with HST and JWST
› Physical Predictions in Closed Quantum Gravity
› Cosmic Ray Spectra and Metal Budget Regulated by the Galactic Wind
› Likelihood-Based One-Class Scoring in CWT Latent Space for Confusion-Limited LISA Gravitational-Wave Detection
› Linking Leptogenesis and Asymmetric Dark Matter: A Testable Framework for Neutrino Mass and the Matter-Antimatter Asymmetry
› Warm dark matter from freeze-in at stronger coupling
› Unitarity violation and restoration in radiative bound-state formation
› Spontaneous particle creation by oscillating compact stars
› A strongly hyperbolic viscous relativistic hydrodynamics theory with first-order charge current
› Electromagnetic Radiation from Cosmic-Ray Scatterings on Relic Neutrinos
› Complex Inflaton Potentials with Nonminimal Coupling: Robust Inflation and Geometric Reheating
› Thermodynamic Gravity with Non-Extensive Horizon Entropy and Topological Calibration
› Range Emulator: A Compact Paraxial Optical System to Emulate Long-Distance Monochromatic Laser Propagation
› Accurate transition and hyperfine data in Ag I from Multiconfiguration Dirac-Hartree-Fock and Relativistic Coupled-Cluster methods
› Gravitational wave radiation from periodic orbits in regular black holes
› 5PN eccentric waveforms for intermediate-mass-ratio-inspirals (IMRIs) from post-Newtonian and black hole perturbation theory
› Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCs
› Investigating the correlations between IceCube high-energy neutrinos and Fermi-LAT $\gamma$-ray observations. II
› Calibrating Bayesian Tension Statistics using Neural Ratio Estimation
› New Constraints on Lorentz Invariance Violation at High Redshifts from Multiband of GRBs
› Cool-Core Destruction in Merging Clusters with AGN Feedback and Radiative Cooling
› Chasing the Light: Shadowing, Collimation, and the Super-Eddington Growth of Infant Black Holes in JWST BLAGNs
› The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science
› A Detection of Circumgalactic Dust at Megaparsec Scales with Maximum Likelihood Estimation
› Neutrinos as a new tool to characterise the Milky Way Centre
› On the accuracy of posterior recovery with neural network emulators
› Exploring the presence of a fifth force at the Galactic Center
› The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies
› Dispu$\tau$able: the high cost of a low optical depth
› DeepVoid: A Deep Learning Void Detector
› Monte Carlo simulations of relativistic shock breakout from a stellar wind
› Insights into the structure and kinematics of a Milky Way-like galaxy
› Non-linear Dynamics and Primordial Black Hole Formation During Kination
› Preferential Positron Acceleration in Relativistic Magnetized Electron-Positron-Ion Shocks
› Simulation-Based Inference for Direction Reconstruction of Ultra-High-Energy Cosmic Rays with Radio Arrays
› High-resolution Giant Metrewave Radio Telescope H{\sc i} 21\,cm imaging of the host galaxy of FRB\,20250316A
› Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes
› Magma ocean interactions can explain JWST observations of the sub-Neptune TOI-270 d
› Feeding the Dead: Neutral Gas Inflow in a Long-Quenched Ancient Massive Galaxy at $z\sim 2.7$ Observed with JWST/NIRSpec
› High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates I. X-ray Coronae
› Clumpy Outflows from Super-Eddington Accreting Black Holes I: Radiation Hydrodynamics Simulations and Observational Implications
› Binding energy of compact stars and their non-radial oscillations
› Assessing the star formation history of all-sky and part-sky 100pc white dwarf samples
› High Resolution (
› Physical properties of long-rising type II supernovae -- Bayesian analytic modeling and spectrophotometric correlations
› Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum
› Modeling Binary Lenses and Sources with the BAGLE Python Package
› First Statistical Detection of MgII-traced Cool Gas Outflows with JWST Towards Cosmic Dawn
› SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope
› The Oxygen Valve on Hydrogen Escape Since the Great Oxidation Event
› Insights for Early Dark Energy with Big Bang Nucleosynthesis
› The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM
› Kinematics of H I and O VI Absorbers: Insights into the Turbulence Driver of the Multiphase Circumgalactic Medium
› Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline
› CLiMB: A Domain-Informed Novelty Detection Clustering Framework for Galactic Archaeology and Scientific Discovery
› Properties and Possible Physical Origins of $\gamma$-ray Emission in Extreme Synchrotron Blazars
› Discovery of Galactic center ejected star in DESI DR1
› Population synthesis of double white dwarfs: evolutionary effects on system properties
› Experimental and numerical modeling of liposome congregation in meteorite craters of Early Earth
› Magnetic structure of coronal dark halos
› SMMAN: quasi-Simultaneous Multi-wavelength Monitoring of gamma-ray-loud AGNs with the Nanshan 26-m radio telescope
› The morphological stability of open clusters: a new 2D perspective
› HelioSpectrotron 5000: An interactive multi-resolution solar spectral atlas
› Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter
› Resolving the QCD Axion Domain Wall Problem with a Light Axion
› Stable Islands of Weak Gravity
› Marginal IR running of Gravity as a Natural Explanation for Dark Matter
› Probing cosmic strings via gravitational-wave lensing
› Equivalence of scalar-tensor theories and scale-dependent gravity
› GraviBERT: Transformer-based inference for gravitational-wave time series

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