Obserwatorium Astronomiczne na Suhorze Strona główna
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Polecamy czytelnikom, nowe wydanie:
J.M.Kreiner - "Ziemia i Wszechswiat"
 Wiadomości z astronet.pl
› XXVI Ogólnopolski Zlot Miłośników Astronomii OZMA 2022 – trwają zapisy!
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› Mity wśród gwiazd: Gwiazdozbiór Oriona
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› W kosmicznym obiektywie: Maraton startów Falcona
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› Mity Wśród Gwiazd: Gwiazdozbiór Małego Psa
RSS  Najnowsze prace na astro-ph:
› A Possible Solution to the Helium Anomaly of EMPRESS VIII by Cuscuton Gravity Theory. (arXiv:2206.11257v1 [gr-qc])
› Cosmological free-free emission from dark matter halos diffuse free-free (background) radiation from dark matter halos. (arXiv:2206.11261v1 [astro-ph.CO])
› Novel neutron decay mode inside neutron stars. (arXiv:2206.11262v1 [hep-ph])
› Equation of state for hot hyperonic neutron star matter. (arXiv:2206.11266v1 [astro-ph.HE])
› Spatially-resolving the terminator: Variation of Fe, temperature and winds in WASP-76 b across planetary limbs and orbital phase. (arXiv:2206.11268v1 [astro-ph.EP])
› Quantum fluctuations masquerade as halos: Bounds on ultra-light dark matter from quadruply-imaged quasars. (arXiv:2206.11269v1 [astro-ph.CO])
› Probable Dormant Neutron Star in a Short-Period Binary System. (arXiv:2206.11270v1 [astro-ph.SR])
› easyFermi: a graphical interface for performing Fermi-LAT data analyses. (arXiv:2206.11272v1 [astro-ph.HE])
› Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations. (arXiv:2206.11274v1 [astro-ph.GA])
› paired: A Statistical Framework for Determining Stellar Binarity with Gaia RVs. I. Planet Hosting Binaries. (arXiv:2206.11275v1 [astro-ph.EP])
› A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension. (arXiv:2206.11276v1 [astro-ph.CO])
› Chandra, HST/STIS, NICER, Swift, and TESS Detail the Flare Evolution of the Repeating Nuclear Transient ASASSN-14ko. (arXiv:2206.11278v1 [astro-ph.HE])
› HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images. (arXiv:2206.11279v1 [astro-ph.IM])
› Analysis of high-resolution FEROS spectroscopy for a sample of variable B-type stars assembled from TESS photometry. (arXiv:2206.11280v1 [astro-ph.SR])
› Sensitivity of Neutron Star Observations to Three-nucleon Forces. (arXiv:2206.11286v1 [astro-ph.HE])
› Silicon Pore Optics. (arXiv:2206.11291v1 [astro-ph.IM])
› Dark Matter Dilution Mechanism through the Lens of Large Scale Structure. (arXiv:2206.11293v1 [hep-ph])
› TangoSIDM: Tantalizing models of Self-Interacting Dark Matter. (arXiv:2206.11298v1 [astro-ph.GA])
› Super-resolution trends in the ALMA Taurus survey: Structured inner discs and compact discs. (arXiv:2206.11308v1 [astro-ph.EP])
› Towards reconstructing the halo clustering and halo mass function of N-body simulations using neural ratio estimation. (arXiv:2206.11312v1 [astro-ph.CO])
› Topography of the Young Galactic Disk: Spatial and Kinematic Patterns of the Clustered Star Formation in the Solar Neighborhood. (arXiv:2206.11313v1 [astro-ph.GA])
› Baryogenesis and Dark Matter in Multiple Hidden Sectors. (arXiv:2206.11314v1 [hep-ph])
› Dissecting the microphysics behind the metallicity-dependence of massive stars radii. (arXiv:2206.11316v1 [astro-ph.SR])
› Surface Properties of Near-Sun Asteroids. (arXiv:2206.11325v1 [astro-ph.EP])
› Undetected Minority-polarity Flux as the Missing Link in Coronal Heating. (arXiv:2206.11327v1 [astro-ph.SR])
› On the relation between duration and energy of non-repeating fast radio bursts: census with the CHIME data. (arXiv:2206.11330v1 [astro-ph.CO])
› Is there a nearby microlensing stellar remnant hiding in Gaia DR3 astrometry?. (arXiv:2206.11342v1 [astro-ph.SR])
› How much metals did the first stars provide to the ultra-faint dwarfs?. (arXiv:2206.11351v1 [astro-ph.GA])
› Computing optical meteor flux using Global Meteor Network data. (arXiv:2206.11365v1 [astro-ph.EP])
› Tidal Heating of Exomoons in Resonance and Implications for Detection. (arXiv:2206.11368v1 [astro-ph.EP])
› Stable lifetime of compact, evenly-spaced planetary systems with non-equal masses. (arXiv:2206.11374v1 [astro-ph.EP])
› Key wavefront sensors features for laser-assisted tomographic adaptive optics systems on the Extremely Large Telescope. (arXiv:2206.11383v1 [astro-ph.IM])
› Metal Lines Associated with the Lyman-alpha Forest from eBOSS Data. (arXiv:2206.11385v1 [astro-ph.CO])
› The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER) II. The Spatially Resolved Recent Star Formation History of M33. (arXiv:2206.11393v1 [astro-ph.GA])
› Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-Prime-Field Planets. (arXiv:2206.11409v1 [astro-ph.EP])
› Solid Accretion onto Neptune-Mass Planets I: In-Situ Accretion and Constraints from the metallicity of Uranus and Neptune. (arXiv:2206.11425v1 [astro-ph.EP])
› Linearity: galaxy formation encounters an unanticipated empirical relation. (arXiv:2206.11431v1 [astro-ph.GA])
› Thermal and non-thermal emission from a peculiar long-duration GRB 211211A. (arXiv:2206.11438v1 [astro-ph.HE])
› Putting Flat $\Lambda$CDM In The (Redshift) Bin. (arXiv:2206.11447v1 [astro-ph.CO])
› RACS2: A Framework of Remote Autonomous Control System for Telescope Observation and its application. (arXiv:2206.11451v1 [astro-ph.IM])
› How Inflationary Gravitons Affect the Force of Gravity. (arXiv:2206.11467v1 [gr-qc])
› Predicting the Geoeffectiveness of CMEs Using Machine Learning. (arXiv:2206.11472v1 [astro-ph.SR])
› Systematically smaller single-epoch quasar black hole masses using a radius-luminosity relationship corrected for spectral bias. (arXiv:2206.11486v1 [astro-ph.GA])
› Synchrotron Self-Compton Afterglow Closure Relations and Fermi-LAT Detected Gamma-Ray Bursts. (arXiv:2206.11490v1 [astro-ph.HE])
› Quasar candidates with periodic variations from the Zwicky Transient Facility. I. Sample. (arXiv:2206.11497v1 [astro-ph.GA])
› Inversions of stellar structure from asteroseismic data. (arXiv:2206.11507v1 [astro-ph.SR])
› Star Formation Activity Beyond the Outer Arm II: Distribution and Properties of Star Formation. (arXiv:2206.11508v1 [astro-ph.GA])
› Star Forming Regions. (arXiv:2206.11512v1 [astro-ph.SR])
› Reconciling Parker Solar Probe observations and magnetohydrodynamic theory: \`a la Kolmogorov vs. \`a la Kraichnan scale-invariance. (arXiv:2206.11514v1 [astro-ph.SR])
› Second-order energy-momentum tensor of a scalar field. (arXiv:2206.11530v1 [gr-qc])
› HORuS transmission spectroscopy and revised planetary parameters of KELT-7b. (arXiv:2206.11548v1 [astro-ph.EP])
› CONCERTO : Digital processing for finding and tuning LEKIDs. (arXiv:2206.11554v1 [astro-ph.IM])
› Dynamics of asteroid systems post rotational fission. (arXiv:2206.11570v1 [astro-ph.EP])
› Gap opening by planets in discs with magnetised winds. (arXiv:2206.11595v1 [astro-ph.EP])
› VISH$\nu$: a unified solution to five SM shortcomings with a protected electroweak scale. (arXiv:2206.11598v1 [hep-ph])
› Starspots Modelling and Flare Analysis on Selected MV Stars. (arXiv:2206.11611v1 [astro-ph.SR])
› Laboratory Experiments on the Radiation Astrochemistry of Water Ice Phases. (arXiv:2206.11614v1 [astro-ph.GA])
› The Nature of Luminous Quasars with Very Large C IV Equivalent Widths. (arXiv:2206.11631v1 [astro-ph.GA])
› Improved binary solution for the gamma-ray binary 1FGL J1018.6-5856. (arXiv:2206.11647v1 [astro-ph.HE])
› V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?. (arXiv:2206.11649v1 [astro-ph.SR])
› Modelling the transport of relativistic solar protons along a heliospheric current sheet during historic GLE events. (arXiv:2206.11650v1 [astro-ph.SR])
› Cosmic-ray electron transport in the galaxy M 51. (arXiv:2206.11670v1 [astro-ph.HE])
› X-ray polarimetry-timing. (arXiv:2206.11671v1 [astro-ph.HE])
› Probing the surface environment of large T-type asteroids. (arXiv:2206.11672v1 [astro-ph.EP])
› Understanding Galaxy Rotation Curves with Verlinde's Emergent Gravity. (arXiv:2206.11685v1 [gr-qc])
› Observational characteristics of radiation-mediated shocks in photospheric gamma-ray burst emission. (arXiv:2206.11701v1 [astro-ph.HE])
› Axion induced angular momentum reversal in Kerr-like black holes. (arXiv:2206.11734v1 [gr-qc])
› The Super-Massive Black Hole close environment in Active Galactic Nuclei. (arXiv:2206.11790v1 [astro-ph.HE])
› A non-linear solution to the $S_8$ tension?. (arXiv:2206.11794v1 [astro-ph.CO])
› Are pulsar halos rare ?. (arXiv:2206.11803v1 [astro-ph.HE])
› An investigation of the magnetic activity of HD 134319 based on TESS photometry and ground-based spectroscopy. (arXiv:2206.11814v1 [astro-ph.SR])
› An uncontaminated measurement of the escaping Lyman continuum at $z\sim3$. (arXiv:2104.02081v2 [astro-ph.GA] UPDATED)
› Constraining Dark Matter Microphysics with the Annihilation Signal from Subhalos. (arXiv:2106.10399v2 [astro-ph.CO] UPDATED)
› Mergers of Maximally Charged Primordial Black Holes. (arXiv:2109.09769v3 [gr-qc] UPDATED)
› Cosmological evolution in Weyl conformal geometry. (arXiv:2110.07056v2 [gr-qc] UPDATED)
› Inverse energy cascade in self-gravitating collisionless dark matter flow and effects of halo shape. (arXiv:2110.13885v2 [astro-ph.GA] UPDATED)
› Polarized Vector Oscillons. (arXiv:2111.08700v2 [astro-ph.CO] UPDATED)
› Phase spirals in cosmological simulations of Milky Way-size galaxies. (arXiv:2111.12414v3 [astro-ph.GA] UPDATED)
› Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates. (arXiv:2201.11088v3 [astro-ph.GA] UPDATED)
› Searching for the connection between ionizing-photon escape and the surface density of star formation at z~3. (arXiv:2202.00016v2 [astro-ph.GA] UPDATED)
› Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices. (arXiv:2202.05949v2 [astro-ph.CO] UPDATED)
› Barrow holographic dark energy with Granda-Oliveros cut-off. (arXiv:2203.14464v2 [gr-qc] UPDATED)
› Signature of primordial non-Gaussianity on 21-cm power spectrum from dark ages. (arXiv:2203.15599v2 [astro-ph.CO] UPDATED)
› Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel. (arXiv:2204.00372v2 [astro-ph.SR] UPDATED)
› Tunnel configurations and seismic isolation optimization in underground gravitational wave detectors. (arXiv:2204.04131v2 [astro-ph.IM] UPDATED)
› Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models. (arXiv:2204.04689v2 [astro-ph.CO] UPDATED)
› Analytical Model of Disk Evaporation and State Transitions in Accreting Black Holes. (arXiv:2204.07495v2 [astro-ph.HE] UPDATED)
› Mergers prompted by dynamics in compact, multiple-star systems: a stellar-reduction case for the massive triple TIC 470710327. (arXiv:2204.10600v2 [astro-ph.SR] UPDATED)
› On the jet-ejecta interaction in 3D GRMHD simulations of binary neutron star merger aftermath. (arXiv:2205.01691v5 [astro-ph.HE] UPDATED)
› Molecular gas dynamics around nuclei of galaxies. (arXiv:2205.06106v2 [astro-ph.GA] UPDATED)
› On the properties of Alfv\'enic switchbacks in the expanding solar wind: three-dimensional numerical simulations. (arXiv:2205.09446v2 [astro-ph.SR] UPDATED)
› The Astrophysical Distance Scale: V. A 2% Distance to the Local Group Spiral M33 via the JAGB Method, Tip of the Red Giant Branch, and Leavitt Law. (arXiv:2205.11323v2 [astro-ph.GA] UPDATED)
› Starobinsky-Bel-Robinson gravity. (arXiv:2205.13172v2 [gr-qc] UPDATED)
› Impact drag force exerting on a projectile penetrating into a hierarchical granular bed. (arXiv:2206.01037v2 [astro-ph.EP] UPDATED)
› Tidally induced spiral arm wraps encoded in phase space. (arXiv:2206.03495v2 [astro-ph.GA] UPDATED)
› The Equilibrium Tide: An Updated Prescription for Population Synthesis Codes. (arXiv:2206.06068v2 [astro-ph.SR] UPDATED)
› Primordial Black Holes and Gravitational Waves in Multi-Axion-Chern-Simons Inflation. (arXiv:2206.07963v2 [hep-th] UPDATED)
› Could the "Wow" signal have originated from a stochastic repeating beacon?. (arXiv:2206.08374v2 [astro-ph.IM] UPDATED)
› Moving Groups Across Galactocentric Radius with Gaia DR3. (arXiv:2206.10633v2 [astro-ph.GA] UPDATED)
› Stringy multifield quintessence and the Swampland. (arXiv:2206.10649v1 [hep-th] CROSS LISTED)

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