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Astronomia w Krakowie
Photo: View to the south-west
View to the south-west
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Temperature
9.6 °C

Humidity
 61%

Wind
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Pressure
1025.5 hPa

Moon

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 News from astronomynow.com

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› Dr Allan Chapman (1946-2026)
RSS  Latest preprints on astro-ph:

› Beyond Cloud-9: The case for discovering more HI-rich failed halos
› The First Empirical Calibration of the MIR Abundance Diagnostic Ne$_{23}$ with JWST
› Coupling between stellar and HI lopsidedness in Milky Way-type galaxies from the Auriga Superstars cosmological simulations
› Unveiling the dynamics of the ultra-fast outflow in IRAS 13224-3809 with X-ray spectroscopy
› Searching for GEMS: Three warm Saturns and a super-Jupiter orbiting four early M-dwarfs
› Dwarf Galaxies Hosting Extreme Star-Forming Regions and (Variable) AGNs at Radio Wavelengths
› SPYGLASS. VII-B. Tracing the Fragments of Massive Star Formation Using Low-Mass Associations
› Chaotic Molecular Gas in Five Dusty Star-forming Galaxies in the Spiderweb Protocluster at $z = 2.16$
› A high-resolution K-band spectral atlas of massive stars
› Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
› Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1
› Geodesically Complete Curvature-Bounce Inflation
› The A Supergiant Eclipsing Binary BM Cas: An Evolved, Intermediate Mass System
› Dust cloud lifetimes of Scallop-shell stars
› uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo
› CORINOS V: Radiative transfer effects in protostellar ice observations
› Molecular Outflows in the Nucleus of the Nearby Compton-thick AGN NGC 3079
› The major cluster merger in Abell 2034 as seen by XRISM: Strong turbulence and spectral anomalies?
› Six New Variable Stars Discovered from Ground-Based Photometry and Characterized with TESS Data
› Formation and Trapping of CO2 from Cryogenic Irradiation of Carbonate
› Iron He-triplet signatures of shocks in the hottest galaxy clusters. Z/W line ratio, line broadening, and electron-ion temperature equilibration
› Multi-messenger emission from choked jets in collapsar
› Turbulence and Star Formation Suppression in Elliptical Galaxies: The Role of Active Galactic Nucleus Jet Wind Interaction
› Extended Universal Rotational Curve of Spiral Galaxies
› Active Galactic Nucleus Feedback in an Elliptical Galaxy. IV. The Importance of the Jet Wind Coupling
› Star cluster formation from turbulent clumps. V. Stellar clustering around massive stars
› The Solar System Notification Alert Processing System (SNAPS): Public access to SNAPS data and products
› A benchmark for binary star interaction with a supermassive black hole in general relativity
› Indication of gamma-Ray Quasi-periodicity in GB6 J1037+5711 from Multi-technique Timing Analysis
› Foreground Mitigation and Power Spectrum Analysis for Tianlai Full-Sky 21 cm Survey Observation
› The Critical Mass in Galaxy Evolution
› First Detection of Faraday Rotation in a Gamma-Ray Burst Afterglow: Low Polarization and High Rotation Measure in GRB 260310A Reveal Jet Magnetic Structure and Environment
› Primordial black hole dark matter from axion inflation
› X-Ray Spectral Variability of the TeV HBL Blazar PG 1553+113 with XMM-Newton
› Detection of optical quasi-periodic oscillation in the blazar 3C 454.3
› Finding Strongly Lensed Supernovae from Blended Light Curves
› Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks
› Dense cores and filaments in M16: Enhanced formation efficiency in the stellar feedback-driven shell
› An Extended Evaluation Split for DeepSpaceYoloDataset
› Diffuse Gamma-ray Emission Around 4FGL J1626.0-4917
› Eclipsing time variations in close binaries produced by azimuthal dynamo waves
› On the Difference Between Pulsar Radio Emission Beams from the Two Poles
› Blazar flares from plasma blobs crossing the broad-line region
› Probing dust properties through polarized scattered-light images of a sample of ring-shaped protoplanetary disks
› Long-term study of the gamma-ray emission of Cygnus X-3 with MAGIC and Fermi-LAT
› Radio signal generation in milliseconds: enabling multi-parameter reconstruction of ultra-high-energy cosmic rays
› A Cosmological Uncertainty Relation and Late-Universe Acceleration
› Robust AGN and host-galaxy decomposition in optical spectral fitting
› TESS Asteroseismology of Red Giants in the Old Metal-Rich Open Clusters NGC 188 & NGC 6791
› Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties
› Anisotropy of Satellite Galaxies-I: Contrasting Correlations with Central Galaxy, Host Halo, and Large-Scale Filament Structures
› Cosmological Observational Tests in the JWST Era. II: The Tolman Test
› Probing the $\gamma$-ray Emission Origin of Two Star-forming Galaxies NGC 2403 and NGC 3424 with the Fermi-LAT
› A New Perspective on Galactic Evolution: Studying the Outskirts of the Abell S1063 Galaxy Cluster
› The Complex Structure of the Abell 548 - Abell 3367 Region
› The Large Array Survey Telescope-Pipeline. II. Image Subtraction and Transient Detection
› Pulsation-driven helium transport as a potential source of the Blazhko effect
› Axion dark matter from extended misalignment with a constant-$\omega_\phi$ pre-oscillatory phase and dark radiation
› Applications of 1.4 GHz diagnostics to Type Ia Supernova host galaxies
› A common four-beam geometry reveals altitude-stratified GeV pulses in canonical young pulsars
› On the polarization position angle jumps in FRB 20240114A
› Cosmological intercept tension
› The faint voice of a radio-weak BL Lacertae: modeling the broadband emission of WISE~J141046.00+740511.2
› Finding the one: identifying the host of compact binary mergers
› The Influences of Hydrogen-Silicate-Iron Miscibility on the Demographics of Sub-Neptunes and Super-Earths
› Chemical Taxonomy of $\omega$~Centauri: Ten Populations Reveal a Multi-Phase Enrichment History
› The intrinsic dispersion of elemental abundance ratios in nearby metal-poor halo stars
› Chiral-Transport-Induced Collective Modes in Strong Magnetic Fields and Their Implications for Neutron Star Phenomenology
› Compressible Navier--Stokes Flow in Schr\"odinger-Type Variables
› Agnostically decoding gravitational wave model deficiencies in GWTC-3
› Stable but Wrong: An Inference Limit in Galactic Archaeology
› Gravitational wave constraints on the Paneitz operator
› Theoretical and Experimental Constraints in the $\mu$--$\tau$ Four-Lepton Sector of the SMEFT: implications to neutrino self interactions
› Stochastic Axion Mixing: A General Mechanism Beyond Decay Constant Constraints
› Rotation-Induced Pressure Anisotropy in Newtonian White Dwarfs: Sequences and Applicability Criteria
› Semi-analytic bounds on axion-like-particle supernovae emission
› New gravitational-wave templates for metastable cosmic strings: Loop breaking versus network collapse
› Beyond the Separatrix: Analytic Continuation of Darwin Variables for Plunging Geodesics in Schwarzschild Spacetime
› Cosmology with Cosmic Voids
› Reconciling Nonminimally Coupled Higgs Inflation with ACT DR6 Observations through Reheating
› 3C403: a candidate neutrino-emitting radio galaxy
› The first radio view of a type Ibn supernova in SN 2023fyq: Understanding the mass-loss history in the last decade before the explosion
› Supernovae drive large-scale, incompressible turbulence through small-scale instabilities
› CosmoGen: A genetic algorithm framework for the exploration of dark energy dynamics
› Adaptive Reconstruction of Cluster Halos (ARCH): Integrating Shear and Flexion for Substructure Detection
› Is the Peculiar Galactic Center Transient Swift J174610.4-290018 A Nova Outburst?
› QML-FAST -- A Fast Code for low-$\ell$ Tomographic Maximum Likelihood Power Spectrum Estimation
› Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations
› Acceleration of Ultrahigh Energy Particles from Fast Radio Bursts
› Niebla: an open-source code for modeling the extragalactic background light
› Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
› Charge-dependent spectral softenings of primary cosmic-rays below the knee
› Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI
› The stellar and dark matter distributions in early-type galaxies measured by stacked weak gravitational lensing
› On the gravitational stratification of multi-fluid-multi-species plasma
› Template-free search for gravitational wave events using coincident anomaly detection
› A Response to paper Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates by Watters et al. (2026)
› NASA's Pandora SmallSat Mission: Simulating the Impact of Stellar Photospheric Heterogeneity and Its Correction
› Broadband Searches for Extraterrestrial Technological Intelligence: a New Strategy To Find Nearby Alien Civilizations
› Post-perihelion Coma Composition of the Interstellar Comet 3I/ATLAS from Optical Spectroscopy
› Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms
› G objects as Primordial Black Hole-Neutron Star Remnants: Population Modeling and Multi-Wavelength Observables
› Observations of DNC and DCO$^+$ toward the $\int$-shaped Filament and Starless Cores in the Orion Molecular Clouds
› Low-mass Active Galaxies in the SAMI Galaxy Survey with Spatially-resolved Spectroscopy
› Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters
› Chemistry and ro-vibrational excitation of CH$^+$ in the planetary nebula NGC 7027
› Stellar feedback SPICEs up [C II] emission in the first galaxies
› Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds
› SCAT Data Release 1: 1810 optical spectra of 1330 transients
› Massive black holes and their galaxies
› Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos
› Blueberry and Green Pea galaxies live in low density environments
› The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars
› Enhancing Early Detection and Localization of Gravitational Waves via Eccentricity-Induced Higher Harmonic Modes with 2G Detector Networks
› Inverting no-hair theorems: How requiring General Relativity solutions restricts scalar-tensor theories
› Axions as Dark Matter, Dark Energy, and Dark Radiation
› Chiral effects and Joule heating in hot and dense matter
› Photon counting readout for detection and inference of gravitational waves from neutron star merger remnants
› A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems
› Massive boson stars: Stability and GW emission in head-on mergers
› Fermion Thermal Field Theory for a Rotating Plasma (with Applications to Neutron Stars)
› Anisotropic dispersion relation of ultralight Bose gases in modified Newtonian dynamics
› Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions
› Warm dark matter from freeze-in at stronger coupling
› Infrared Spectral Gap in a Gluonic Dark Sector as the Origin of the Galactic Acceleration Scale
› Boson star-black hole binaries: initial data and head-on collisions
› Investigating the Neutrino Mass Ordering Problem via Ternary Plots

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