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Astronomia w Krakowie
Photo: view from south-west
view from south-west
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 92%

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Pressure
1016.2 hPa

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Moon

 News from astronomynow.com
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
› Binoculars to boost your night-sky viewing
› Lyra’s stunning smoke ring – M57
› Is the Hubble Tension Resolved?
› Universe’s end – sooner rather than later
RSS  Latest preprints on astro-ph:
› The Interpolation Constraint in the RV Analysis of M-Dwarfs Using Empirical Templates
› Towards high-precision inspiral gravitational waveforms from binary neutron star mergers in numerical relativity
› The extended molecular gas of the Circinus galaxy and NGC 1097 as seen by APEX
› White dwarf-neutron star binaries: a plausible pathway for long-duration gamma-ray bursts from compact object mergers?
› Supernova Rates and Luminosity Functions from ASAS-SN II: 2014-2017 core-collapse supernovae and their subtypes
› Population III star formation near high-redshift active galactic nuclei
› A massive, evolved slow-rotating galaxy in the early Universe
› The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star
› An Ultraviolet Study of CO Chemistry in the Magellanic Clouds
› $r$-process Abundance Dispersion in the Globular Cluster M5 using Keck Archival Data
› Not-so-heavy metal(s): Chemical Abundances in the Ultra-faint Dwarf Galaxies Eridanus IV and Centaurus I
› Three dimensional magnetic reconnection mediated with plasmoids and the resulted multi-thermal emissions in the cool atmosphere of the Sun
› JWST NIRCam Imaging of NGC 4258: I. Observation Overview
› Explosions of pulsating red supergiants: a natural pathway for the diversity of Type II-P/L supernovae
› Four binary microlenses with directly measured masses
› Pulsations change the structures of massive stars before they explode: interpreting the nearby supernova SN 2023ixf
› First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b
› Developments on LLNL's high contrast testbed and Lick/ShaneAO
› SQ-A: A Collision Triggered Starburst in Intra-Group Medium of Stephan's Quintet
› Discovery of H$\alpha$ Emission from a Protoplanet Candidate Around the Young Star 2MASS J16120668-3010270 with MagAO-X
› NGC 2392 and NGC 4361: Spectroscopic Diagnostics of Planetary Nebula Evolution
› Demonstrating the velocity response of a table-top EPR Speedmeter
› High-Resolution Simulations of the Interaction Between the Nova/Supernova Ejecta and the Accretion Disk
› The Mass of Cosmic Rays of Ultra High Energy
› JWST/MIRI Observations of PAH Emission and Evolution in H II Regions of NGC 5457
› Improving Air Shower Simulations by Tuning Pythia 8/Angantyr with Accelerator Data
› Search of RRATs on declinations from $+42^{\circ}$ to $+55^{\circ}$ with a neural network
› Pair Cascades in Magnetar Magnetospheres
› SN 2021aaev: a Hydrogen-Rich Superluminous Supernova with Early Flash and Long-Lived Circumstellar Interaction in an Unusual Host Environment
› Propagation of Precessing Jet in Envelope of Tidal Disruption Events
› Breaking the Strings: the signatures of Cosmic String Loop Fragmentation
› Bulk viscous cosmological models with cosmological constant: Observational constraints
› Polarized Emission of Intrabinary Shocks in Spider Pulsars from Global 3D Kinetic Simulations
› Shedding light on dark matter spikes through neutrino-dark matter interactions
› Cooling of quark stars from perturbative QCD
› Inference with finite time series II: the window strikes back
› Bridging the Gap between Collisional and Collisionless Plasma Shocks: A Simulation Study using OSIRIS
› Theoretical Detailed Analyses for DC readout and a Fabri-P\'erot gravitational-wave detector
› The NHIM development scenario in an asymmetric binary system of dwarf galaxies
› Probes for String-Inspired Foam, Lorentz, and CPT Violations in Astrophysics
› The DeepFMKit Python package: A toolbox for simulating and analyzing deep frequency modulation interferometers
› Extra-natural production of superheavy Kaluza-Klein particles
› Nambu-Goldstone boson phenomenology in Domain-Wall Standard Model
› ACT inflation and its influence on reheating era in Einstein-Gauss-Bonnet gravity
› Laser Interferometer Lunar Antenna (LILA): Advancing the U.S. Priorities in Gravitational-wave and Lunar Science
› Probing vector chirality in the early Universe
› Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale
› A new way to find symbiotic stars: accretion disc detection with continuum survey photometry
› Spatial models of r-process remnants and their gamma-ray detectability
› Discovery and Multi-Wavelength Analysis of a New Dissociative Galaxy Merger: The Champagne Cluster
› The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
› Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
› EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
› Modelling Gaia photometry signals of dark halos
› The morphology of supernova remnant G0.9+0.1 implies explosion by jittering-jets
› Tomographic Alcock-Paczynski Test with Marked Correlation Functions
› Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition
› Convolutional Autoencoders for Data Compression and Anomaly Detection in Small Satellite Technologies
› Primordial black hole-star binaries via dynamical friction
› Revealing the nature of long period transients with space-based gravitational-wave interferometers
› Observing Supernova Neutrino Light Curves with Super-Kamiokande.VI. A Practical Data Analysis Technique Considering Realistic Experimental Backgrounds
› CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
› The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8$-$1613
› What drives the growth of black holes: a decade of progress
› Milliarcsecond astrometric oscillations in active galactic nuclei as a precursor of multi-messenger gravitational wave events
› Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods
› Prior-free cosmological parameter estimation of Cosmicflows-4
› A New Method for Measuring the Pion-Air Cross Section at Multi-TeV Energies Using Muon Bundle Properties in Deep Underground Detectors
› Revealing the Origins of Galactic Globular Clusters via Their Mg-Al Abundances
› Daily fluctuations propagate damply through the accretion disk of Swift J1727.8-1613
› Strong NUV Refractory Absorption and Dissociated Water in the Hubble Transmission Spectrum of the Ultra Hot Jupiter KELT-20 b
› Macroscopic approaches to rotating neutron stars
› The Dark Energy Bedrock All-Sky Supernova Program: Cross Calibration, Simulations, and Cosmology Forecasts
› White Dwarf Structure and Binary Inspiral Gravitational Waves from Quantum Hadrodynamics
› Shadows of generalised Hayward spacetimes : in vacuum and with plasma
› Supercooled phase transitions in conformal dark sectors explain NANOGrav data
› Exploring sub-GeV dark matter via $s$-wave, $p$-wave, and resonance annihilation with CMB data
› Doubly regular black holes
› Challenging a binary neutron star merger interpretation of GW230529

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