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:

› Mars, a Post-Habitable Planet?
› The role of the Hubble Space Telescope in advancing our understanding of atmospheric escape in exoplanets
› From Hubble to HWO: Bridging the Frontier of White Dwarf Exoplanet Science
› Exploring Space Weather From Young Solar-like Stars as Windows to Exoplanetary Habitability
› White dwarf planetary systems in the ultraviolet
› Bimodality in Rotational Modulation of Planet-Hosting Stars
› A framework for modelling Population III stars in cosmological simulations
› How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function
› Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps
› NISER-IUCAA New Simulations of JWST GAlaxies and Quasars(NINJA): Properties of galaxies at $5 \leq z \leq 10$
› The Persistent Missing Mass Problem in Planet Formation
› Dynamical Stability and Habitability in the HD 20794 System
› Strong Constraints on Millisecond Pulsar Injection Spectra from Fermi-LAT Observations of the Galactic Center
› Limited imprint of high-mass IMF variations on sodium abundances in main-sequence galaxies
› Bar-halo interaction: the role of orbital anisotropy
› Constraining Scattering Medium Geometry with Cyclic Spectroscopy
› Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in \tigresspp\ Simulations
› NuSTAR as an Axion Helioscope: probing axion-nucleon and axion-electron couplings
› Nuclear Physics of Binary Neutron Star Mergers
› A distributed resource-adaptive implementation of the widefield radio-interferometric measurement model for scalable image formation
› The Role of Whistler and Ion Cyclotron Waves in Particle Escape from Mirror Modes in the Intracluster Medium
› Inversion of CHASE H$\alpha$ Spectral Line during Solar Flares Based on RADYN Dataset via Deep Learning
› An SMA Molecular Inventory of the Edge-on Protoplanetary Disk Gomez's Hamburger
› Unveiling the dark matter nature with reionization relics
› Constraining the Supernova Remnant Environment of FRB 190520B with Dispersion Measure and Scattering Timescale
› A Modified Multi-Level Tracking Scheme for the Detection of Sunspot Umbral Dots
› The DECam MAGIC Survey $-$ Mapping the Ancient Galaxy in CaHK: Overview and Summary of Early Science
› OH/IR stars in the inner Galactic bulge: I. Colour, CO line, and stellar light curve characteristics
› Spectra and Ionization Efficiencies of Charged Decay Particles in Kilonova Ejecta
› Detection of the distant quasar OP 313 with the first Large-Sized Telescope of CTAO
› From supernovae to neutron stars: crust formation time
› Interior-Atmosphere Coupling on TRAPPIST-1 f, g, and h: Cryovolcanic Water Exospheres and Infrared Detectability
› Invariant manifolds in barred galaxy simulations. II. Quantitative evidence of manifold-trapping in spiral arm formation
› Evidence for Systematically Larger Dust Grains in Upper Scorpius Relative to Taurus Disks
› Granulation signatures as seen by Kepler short-cadence data. II. A hierarchical route to inferring stellar radii from granulation
› Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis
› From streamers to stars: overcoming mass loss in protoplanetary disks
› The spectral energy distribution of YSES 1 b and its circumplanetary disc
› Magnetic field Topology and Star Formation in the Cepheus B Filamentary cloud under External Feedback
› Survival of very small carbonaceous dust grains in the inner-CGM of NGC 891 from JWST/MIRI MRS
› Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena
› The Baryonic Faber-Jackson Relation and Fundamental Plane of Galaxy Groups, Elliptical Galaxies, and Dwarf Galaxies
› Veiling of Photosphere Lines in the Spectra of UX ORI Stars at Deep Light Minima. I. The Star RR Tau
› The small transiting planet population revealed by ESPRESSO with extreme precision radial velocities
› The Physical Nature of Regolith on Icy Moons
› The Simons Observatory: Rotation Performance of Cryogenic Half-Wave Plate Polarization Modulators
› Analysis of Short-term Solar Activity Variability and Estimating the Timings of the Next Enhanced Bursts
› Destructuring the disk of AB Aurigae: Dynamics and accretion
› Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys
› Observations of stable pickup He$^+$ tori in a magnetic flux rope at 0.85 au
› Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster. VI. A star-forming UDG in Hydra I: a rare UDG or a transition phase?
› Nearby galaxies in the LOFAR Two-metre Sky Survey IV. A fundamental plane of the radio-SFR relation
› The pollution from massive AGB stars favoured by strong hot bottom burning
› Regular black hole solutions and the quark chemical potential at the QCD phase transition
› Digging into the Massive Protostar S255IR NIRS3: A Study of Nitrogen-Bearing Molecules and Their Prebiotic Chemistry
› For modified gravity, it's the LITTLE THINGS that matter
› Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
› GWTC-5.0: Population Properties of Merging Compact Binaries
› GWTC-5.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation
› $w_0$-probe: A new diagnostic of dark energy based on $Om$
› A Fast Method to Compute Scalar Induced Gravitational Waves on a Lattice with Primordial Non-Gaussianities
› The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization
› Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae
› Heavy element enrichment of gas in surface-accretion disks: A possible origin of the mass-metallicity anti-correlation in exoplanets
› The Neptunian ridge planet WASP-156 b does not have a polar orbit
› Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply
› Supermassive Black Holes: modelling strongly and weakly magnetised misaligned accretion disks
› Impact of Clouds on the Atmosphere-Mantle Interface of Sub-Neptunes
› Gaussian Process Reconstruction of Cosmological Parameters with Gravitational Wave Sirens using Machine Learning
› Hot Jupiters' Isolation Is Not Unique to High-Eccentricity Tidal Migration
› The first near-infrared high-resolution \'echelle spectroscopy of the outflow in NGC 4151. A study of the clouds covering the Eye of Sauron
› A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS
› First Light and Reionization Epoch Simulations (FLARES) XXII: UV-dust spatial offsets at the Epoch of Reionisation
› Inflatable devices for planetary aerocapture and aerobraking manoeuvres
› Electromagnetic Signatures From Primordial Black Holes in the Solar System
› Charging Across the Phantom Divide with Modified Gravity
› Energy extraction from NED-deformed rotating black holes via the Comisso-Asenjo reconnection process
› Improved Big Bang Nucleosynthesis constraints on decaying massive relics
› Looking for Condensed Gluons: A Cross-Scale Journey from the Deep Structure of Protons to High-Energy Cosmic Rays -- A Mini-Review
› Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run
› Hybrid Expansion Cosmology in f(T) Gravity: Late-Time Evolution and Observational Bounds
› GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog
› GWTC-5.0: Methods for Identifying and Characterizing Gravitational-wave Transients
› GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
› Strong-lensing degeneracies of black holes embedded in self-interacting scalar field dark matter halos
› HAMSTER: Hyperspectral Albedo Maps dataset with high Spatial and TEmporal Resolution
› Exploring Galactic open clusters with Gaia. II Dynamical Evolution and Stellar Population Properties in Fifteen Nearby Open Clusters
› Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
› Co-evolution of cosmic ray energy spectra, composition, and anisotropies
› Relativistic accretion and burdened primordial black holes
› Echoes in Different Tempo: Long-Term Monitoring of Crab Echoes with CHIME
› A Melody in the Noise: Modeling Echoes of the Crab Nebula
› X-ray polarization of reflected thermal emission
› Properties of cluster red-sequence spiral galaxies
› Deciphering the explosion mechanism of Type Ia SNe using their remnants II: a deep dive into double detonations with SNR 0509-67.5
› TOI-2155 b: A Massive Brown Dwarf or a Very Low-Mass Star?
› ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution
› On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
› Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet
› Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission
› Episodic planetesimal disruptions triggered by dissipation of gas disk
› ODIN: Clustering Properties of Ly$\alpha$ Blobs at $z$ $\sim$ 2.4 and 3.1
› Democratic heliocentric coordinates underestimate the rate of instabilities in long-term integrations of the Solar System
› The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs
› LISA and the LISA Science Team
› On the rotation of M-type asteroids: statistical evidence for higher rotation rates
› Direct simulations of H-He mixtures at planetary interior conditions: demixing, insulator-metal transition and miscibility boundaries
› Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth
› IGR J12580+0134: A Possible Repeated Partial Tidal Disruption Event Inferred from Late-Time Radio Re-brightenin
› You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei
› Multimessenger Characterization of High-Energy Neutrino Emission from the Brightest Neutrino-Active Galactic Nuclei
› Inflation with the Gauss-Bonnet term in the Palatini formulation
› Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength
› Dynamical Systems in Cosmology: Reviewing An Alternative Approach
› Exploring the interplay of late-time dynamical dark energy and new physics before recombination
› The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
› Emergence of Complex Web Structures
› Breaking Free from the Swampland of Impossible Universes through the DESI Portal
› Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH mapping along the Orion BN/KL explosive outflow and irradiated shocks
› Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference
› Rotation-curve residuals reveal a suppressed acceleration branch in dwarf galaxies
› Performance analysis of extragalactic classifications in Gaia Data Release 4
› Nature of HD 251108: an RS CVn binary with a long-term evolving spot
› HiFAST: An HI data calibration and imaging pipeline for the FAST IV: The stray-radiation correction
› The Evolution of Cataclysmic Variables Under Various Magnetic Braking Prescriptions
› Reassessing high-energy emission correlations in gamma-ray bursts using a large, homogeneous sample of X-ray afterglows
› Core-collapse supernovae and supernova neutrinos
› Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves
› Examining the influence of anisotropy on the fundamental mode of nonradial oscillation in neutron stars on a complete general relativistic scheme
› Ultralight Dark Matter from the Edge of Field Space
› Semi-convection in rotating spherical shells: flows, layers and dynamos
› Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
› AI-based separation of turbulence from coherent background flows in decaying hydrodynamic turbulence
› Numerical simulations of primordial black hole formation via delayed first-order phase transitions
› High-power Test and System Integration of Direct RF Sampling Based LLRF Control and Monitoring System for S-Band Accelerating Structures
› Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations
› Quantification of atmospheric carbon dioxide from the Geostationary Operational Environmental Satellite (GOES East)
› Aurora Hunter: A Two-Stage Framework for Probabilistic Visibility Forecasting

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