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Astronomia w Krakowie
Photo: Zorza polarna 10 maja 2024
Zorza polarna 10 maja 2024
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Temperature
13.4 °C

Humidity
 65%

Wind
4.8 km/h

Pressure
1025.1 hPa

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 News from astronomynow.com

› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
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› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
› XRISM solves gamma-Cas’s 50-year X-ray mystery
RSS  Latest preprints on astro-ph:

› Deconstructing Sunlight - A Community Enterprise
› Which is the best day of the week to submit to arXiv:astro-ph?
› Full-Covariance Bayesian Inference of Stochastic Gravitational Wave Background with Time-Domain Simulations for Taiji-like Missions
› Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory
› A new measurement of the FRB DM-galaxy cross correlation and a first joint analysis with the kinematic SZ effect
› ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo
› A Diverse Distribution of Black Hole Spins from Stable Mass Transfer
› Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet. A parameter study in locally isothermal discs
› XRISM Spectroscopy of Variable Accretion-driven Disk Winds in NGC 4151: When, Where, and How Fast Outflows are Launched
› A Pair of Warm Saturn-mass Planets near the 2:1 Mean Motion Resonance around TOI-3850
› Spectral Energy Distribution Analysis for Habitable Worlds Observatory Target Stars
› From blue to red spirals: Slow galaxy transformation via ram pressure stripping in TNG-50
› Long-duration GW Searches for Sub-solar NSs and Superkilonovae using CoCoA
› Magnetic fields in extreme primordial halos: turbulent collapse and implications for early quasar formation
› Solar-Cycle Modulation and Photospheric Magnetic Control of Turbulence in the Young Solar Wind
› Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array
› Numerous bow shocks in the outer Helix Nebula
› Chemistry here and there: Comparison between the CMZ of the Milky Way and NGC 253
› A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution
› Testing Covarying Coupling Constants (CCC) against the full SPARC rotation-curve sample: a like-for-like comparison with MOND and NFW
› Dynamic Trajectory Analysis of Meteoroids Showing Minimal Deceleration
› A Radiation-Hydrodynamic Light Curve Grid and Interpolation Framework for Stripped-Envelope Supernovae
› Towards Genuine Coexistence: Per-Satellite Emission and Radiation Limits to Protect Radio Astronomy and Geodetic VLBI at 1-14 GHz from Satellite Constellations
› Disco in the Dust: Reflected light at the bow shock around Betelgeuse's companion explains its observed luminosity
› LIGO A$^\sharp$: Detector Design and Science Prospects Beyond A+
› Altered Cosmic Organics as Venus' Ultraviolet Absorbers
› Molecule-specific diffusion and desorption of interstellar ices on carbonaceous dust
› Cherenkov light as a mechanism for light flashes seen by astronauts in space
› Radio flares and X-ray hardening embedded in the long soft state of 4U 1543-475
› Infrared-to-visible albedo ratio of Phobos: Comparison with primitive asteroids
› Statistics of Solar Filament Mass based on CHASE Sun-as-a-star Spectroscopic Observations
› Results from the first spectropolarimetric survey of $\gamma$ Dor pulsators
› SPORE: An Event-Level Sampling Pipeline for Multi-Telescope Neutrino Astronomy
› Chemical Tracers for 3D Atmospheric Asymmetries on WASP-69 b
› First and Comprehensive Study of V0757 Pup : $\gamma-$Doradus Pulsator in Detached Eclipsing Binary
› Three new exoplanet systems from the Dispersed Matter Planet Project
› 1.5D investigation of the Hanle effect in the Ca I 4227 line using partial frequency redistribution. Comparison of synthetic Stokes profiles in Bifrost and MURaM-ChE rMHD models
› Classifying Quasar Types Without a Spectrum
› Chemical fingerprints of binary mass transfer in massive stars
› New constraints on the binary system HD 327083 and its gaseous and dusty environments
› Discovery of 27 new Rotating Radio Transients by MeerTRAP
› Spiral structure from the interference of gravitational eigenmodes in ultralight dark matter halos
› Deep MUSE observations of SNR 0509-67.5 reveal a double degenerate merger progenitor
› Evolutionary tracks of giant planets formed by disk instability
› Identification of a Large-Scale Diffuse Gamma-Ray Structure in the Southern Galactic Hemisphere
› Constraining the gamma-ray efficiency of LINER outflows with Fermi-LAT and MEGARA
› Search for a Globular Cluster whose Passage through the Galactic Disk could Trigger the Radcliffe Wave
› Automation and Modernisation of Legacy BiSON Solar Observatories with the BiSON:NG Platform
› MeerKAT Reveals Evidence of a Radio Megahalo at GHz Frequency
› Updates to WFC3/UVIS Encircled Energy Values in Select Filters
› CIBER $\times$ galaxy cross-correlations reveal a bright, low-redshift NIR background
› The effect of galaxy interactions on star formation rates in the COLIBRE simulations
› Voltage-to-temperature calibration of the High Altitude THz Solar telescope acquisition system
› The Shape of the Vertical Action Distribution Locates the Scatterers that Heat the Galactic Disc
› Impact of Neutrino Flavour Conversion on the Diffuse Neutrino Background from Neutrino-dominated Accretion Flows
› Nascent Embedded-protostar Survey in Taurus (NEST) I: Protostellar Multiplicity
› LIGO Detector Characterization in the Second and Third Parts of the Fourth Observing Run
› High-energy neutrino signatures of embedded GRB jets in AGN disks: a dynamic jet-propagation framework
› Evidence for the First Globular Cluster Stellar Stream beyond the Milky Way
› A systematic comparison of green valley selection criteria across multiparameter spaces using a homogeneous ultraviolet-optical dataset
› The Delay Time Distribution of Quasi-Periodic Eruptions
› Hemispheric Asymmetry of Solar Active Regions Arises from a Nested Population
› CHANG-ES XL: Magnetic Field Structures in the Disk and Halo of NGC 891
› From Cluster Cores to the Low-Density Field: Strong Environmental Quenching of Galaxy Star Formation at Low Redshift
› Radiative Signatures from Warp Drives Traveling Through the Earth's Atmosphere
› A Dynamical-Photometric Phase Space for Spiral Galaxies: Probing the Local Coupling Between Light and Gravity
› Torsional pseudo-inflation beyond Einstein-Cartan
› Constraints on ultralight bosons from merging binary and remnant black holes observed during the second and third parts of the fourth LIGO-Virgo-KAGRA observing run
› Taiji Resolving Power for the Transverse Scalar Mode of Gravitational Waves
› The Ambipolar electric field in multispecies plasma atmospheres: effects of alpha particles and stochastic heating
› Transport properties in binary neutron star mergers: Effect of magnetic field
› Robustness of the primordial power spectrum in hybrid loop quantum cosmology to approximations near the bounce
› PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
› Multiprobe cosmology forecasts from halo-occupation-distribution-based forward modeling of galaxy and void statistics
› Deciphering The Launching of Multi-phase AGN-driven Outflows and Their (Spatially Resolved) Multi-scale Impact
› Dynamical Evolution of Quasi-Hierarchical Triples
› Analysis of the plane of satellites around Milky Way- mass galaxies in the IllustrisTNG simulation
› Robust magnetic field estimates in star-forming galaxies with the equipartition formula in the absence of equipartition
› An Investigation of Systematic Effects from Background Priors on PSR J0740$+$6620 Radius Estimates using Synthetic NICER and XMM-Newton Data
› Equivalence of Stability Criteria for Multi-Fluid Stars
› Widespread Extended [CII] Emission in High-Redshift Galaxies: Insights from the FIRE-2 Cosmological Zoom-in Simulations
› Electron-positron cascade in magnetospheres of supermassive Kerr black holes and the origin of relativistic AGN jets
› Synchrotron self-Compton process for constraining sub-GeV dark matter in Omega Centauri via SKA
› Analytical Estimates of Gravitational Wave Background Anisotropies from Shot Noise and Large-Scale Structure in Pulsar Timing Arrays
› Addressing the Impact of Solar Modulation Systematic Uncertainties on Cosmic-Ray Propagation Models
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion
› Introducing sapphire: Towards Hybrid Physics-Informed, Data-Driven Modeling of Galaxy Formation
› Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing
› Ionization Structure and Metal Enrichment of the Galactic Center Minispiral Observed with JWST
› Systematic KMTNet Planetary Anomaly Search. XIII. Complete Sample of 2021 Prime Field Planets
› Giant impact between high-viscosity Theia and low-viscosity proto-Earth: Origin of lunar isotopic crisis
› Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
› ALMA visits the QSO MUSEUM: Connecting molecular gas and the cool circumgalactic medium around 37 z~3 quasars
› Electron Densities of Typical Low-Mass Galaxies at z~2-7 from Stacked JWST/NIRSpec Spectra
› Unveiling the Nature of C/2023 A3 (Tsuchinshan-ATLAS): A Multi-Technique Observational Approach
› Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry
› A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction
› CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies
› Parametric Study of Torus Instability Threshold
› Electron temperature and emission measure of HII regions in the central molecular zone (CMZ) from H40 \alpha recombination line and continuum emissions by ALMA CMZ Exploration Survey - ACES -
› The Radcliffe Wave is not alone in the Local System
› Gravity modes and potential evidence for Rossby Waves in late O-type supergiants
› Signature of axion dark matter in low-frequency terrestrial electromagnetic fields: formulation and predictions
› Gravity and the Hierarchy Problem
› Impact of higher-order modes on eccentricity measurement in binary black hole gravitational waves
› Structured generalized sliced Wasserstein distance for keV X-ray polarization analysis with Gas Pixel Detector
› ACT-Planck data and phase transitions from a viable no-scale Standard Model completion
› Rotation of the polarization plane in axion fields: application to neutron star polar cap regions
› Exact general relativistic solutions for a cylindrically symmetric stiff fluid matter source

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