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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Instytut Fizyki UP
Astronomia w Krakowie
Zdjecie: ponad chmurami
ponad chmurami
Cloud conditions

Chmury

Rain conditions

Opady

Allsky

Niebo

Temperatura
-2.7 °C

Wilgotność
 88%

Wiatr
11.3 km/h

Ciśnienie
1018.3 hPa

Moon

Księżyc

Polecamy czytelnikom, nowe wydanie:
J.M.Kreiner - "Ziemia i Wszechswiat"
 Wiadomości z astronet.pl
› W kosmicznym obiektywie: Kolebka gwiazd w podczerwieni
› Kosmologia 2: Znajdowanie odległości w kosmosie
› JWST posłuży dwa razy dłużej
› Mity wśród gwiazd: Gwiazdozbiór Herkulesa
› Trwa konkurs Cosmic Challenge dla uczniów szkół podstawowych i ponadpodstawowych
› W kosmicznym obiektywie: Niebo nad ALMA
› Mity wśród Gwiazd: Gwiazdozbiór Korony Północnej
› W kosmicznym obiektywie: Worek Węgla
› Podsumowanie 2021 roku w astronomii
› Tajemnica chemicznie różnych gwiazd w układach podwójnych
RSS  Najnowsze prace na astro-ph:
› Can dark energy emerge from a varying $G$ and spacetime geometry?. (arXiv:2201.04629v1 [gr-qc])
› Shocked jets in CCSNe can power the zoo of fast blue optical transients. (arXiv:2201.04636v1 [astro-ph.HE])
› Weighing the Galactic disk using phase-space spirals IV. Tests on a 3d galaxy simulation. (arXiv:2201.04637v1 [astro-ph.GA])
› Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE. (arXiv:2201.04641v1 [astro-ph.GA])
› An Exomoon Survey of 70 Cool Giant Exoplanets and the New Candidate Kepler-1708 b-i. (arXiv:2201.04643v1 [astro-ph.EP])
› Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations. (arXiv:2201.04644v1 [astro-ph.GA])
› First detection of a magnetic field in low-luminosity B[e] stars: New scenarios for the nature and evolutionary stages of FS CMa stars. (arXiv:2201.04645v1 [astro-ph.SR])
› The Rate, Amplitude and Duration of Outbursts from Class 0 Protostars in Orion. (arXiv:2201.04647v1 [astro-ph.SR])
› The recent LMC-SMC collision: Timing and impact parameter constraints from comparison of Gaia LMC disk kinematics and N-body simulations. (arXiv:2201.04648v1 [astro-ph.GA])
› Locating the CSM Emission within the Type Ia Supernova Remnant N103B. (arXiv:2201.04653v1 [astro-ph.HE])
› Neutrino effective potential in a fermion and scalar background in the resonance region. (arXiv:2201.04661v1 [hep-ph])
› The Fundamental Planes of Black Hole Activity for Radio-Loud and Radio-Quiet Quasars. (arXiv:2201.04666v1 [astro-ph.HE])
› Towards a Dark Sector Model from String Theory. (arXiv:2201.04668v1 [hep-th])
› Optical Photometry of WR140 as the Dust Formed During the 2016 Periastron Passage. (arXiv:2201.04670v1 [astro-ph.SR])
› The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) : I. Characterisation of extended Lyman-alpha haloes and spatial offsets. (arXiv:2201.04674v1 [astro-ph.GA])
› Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator. (arXiv:2201.04679v1 [astro-ph.CO])
› AGN in the ULIRG HE 0435-5304. (arXiv:2201.04685v1 [astro-ph.GA])
› Comparison between core-collapse supernova nucleosynthesis and meteoric stardust grains: investigating magnesium, aluminium, and chromium. (arXiv:2201.04692v1 [astro-ph.SR])
› The synchrotron mechanism and the high energy flair from PKS 1510-089. (arXiv:2201.04693v1 [astro-ph.GA])
› Let the Great World Spin: Revealing the Stormy, Turbulent Nature of Young Giant Exoplanet Analogs with the Spitzer Space Telescope. (arXiv:2201.04711v1 [astro-ph.EP])
› Partial-Attribution Instance Segmentation for Astronomical Source Detection and Deblending. (arXiv:2201.04714v1 [astro-ph.IM])
› The 3D magnetic field morphology of the Perseus molecular cloud An arc-shaped morphology. (arXiv:2201.04718v1 [astro-ph.GA])
› Ground-based gamma-ray astronomy: history and development of techniques. (arXiv:2201.04719v1 [astro-ph.IM])
› The Road to Precision Cosmology. (arXiv:2201.04741v1 [astro-ph.CO])
› Study of changes in the pulsation period of 148 Galactic Cepheid variables. (arXiv:2201.04748v1 [astro-ph.SR])
› FGC 1287 and its enigmatic 250 kpc long HI tail in the outskirts of Abell 1367. (arXiv:2201.04763v1 [astro-ph.GA])
› Data Pipeline Architecture and Development for VELC onboard Space Solar Mission AdityaL1. (arXiv:2201.04863v1 [astro-ph.IM])
› Detection of Gravity Modes in RR Lyrae Stars. (arXiv:2201.04869v1 [astro-ph.SR])
› Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales. (arXiv:2201.04887v1 [astro-ph.CO])
› Large Interferometer For Exoplanets (LIFE): VI. Ideal kernel-nulling array architectures for a space-based mid-infrared nulling interferometer. (arXiv:2201.04891v1 [astro-ph.IM])
› Strong [OIII]{\lambda}5007 emission line compact galaxies in LAMOST DR9: Blueberries, Green Peas and Purple Grapes. (arXiv:2201.04911v1 [astro-ph.GA])
› Dark radiation constraints on light primordial black holes. (arXiv:2201.04946v1 [astro-ph.CO])
› Symmetries in Stellar, Galactic and Extragalactic Astronomy. (arXiv:2201.04966v1 [physics.pop-ph])
› Radio bridges of the future between Solar system and the nearest 50 stars. (arXiv:2201.04969v1 [physics.pop-ph])
› Small-scale magnetic fields of the spectroscopic binary T Tauri stars V1878 Ori and V4046 Sir. (arXiv:2201.04978v1 [astro-ph.SR])
› Reconstruction of dark energy density by non-parametric approaches. (arXiv:2201.04993v1 [astro-ph.CO])
› B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main. (arXiv:2201.05059v1 [astro-ph.GA])
› Is magnetically dominated outflow required to explain GRBs?. (arXiv:2201.05062v1 [astro-ph.HE])
› Feeding the spider with carbon -- [CII] emission from the circum galactic medium and active galactic nucleus. (arXiv:2201.05064v1 [astro-ph.GA])
› Probing the circumgalactic medium with CMB polarization statistical anisotropy. (arXiv:2201.05076v1 [astro-ph.CO])
› A search for ionised gas outflows in an Halpha imaging atlas of nearby LINERs. (arXiv:2201.05080v1 [astro-ph.GA])
› Martian Dust Storms and Gravity Waves: Disentangling Water Transport to the Upper Atmosphere. (arXiv:2201.05081v1 [astro-ph.EP])
› Modeling the hydrological cycle in the atmosphere of Mars: Influence of a bimodal size distribution of aerosol nucleation particles. (arXiv:2201.05086v1 [astro-ph.EP])
› Insights into the evolution of five isolated galaxies. (arXiv:2201.05090v1 [astro-ph.GA])
› The BepiColombo solar conjunction experiments revisited. (arXiv:2201.05107v1 [gr-qc])
› Comments on the mass sheet degeneracy in cosmography analyses. (arXiv:2201.05111v1 [astro-ph.CO])
› PDRs4All: A JWST Early Release Science Program on radiative feedback from massive stars. (arXiv:2201.05112v1 [astro-ph.GA])
› Star formation near the Sun is driven by expansion of the Local Bubble. (arXiv:2201.05124v1 [astro-ph.GA])
› New Options for SUSY-kind Dark Matter. (arXiv:2201.05127v1 [hep-ph])
› Fully Adaptive Bayesian Algorithm for Data Analysis, FABADA. (arXiv:2201.05145v1 [astro-ph.IM])
› Unresolved Binaries in the Intermediate Mass Range in the Pleiades Star Cluster. (arXiv:2201.05146v1 [astro-ph.SR])
› FRAMEx II: Simultaneous X-ray and Radio Variability in Active Galactic Nuclei $-$ The Case of NGC 2992. (arXiv:2201.05152v1 [astro-ph.GA])
› Spectral Variability of VHS J1256-1257 b from 1 to 5 $\mu$m. (arXiv:2004.05168v3 [astro-ph.EP] UPDATED)
› Conservative, density-based smoothed particle hydrodynamics with improved partition of the unity and better estimation of gradients. (arXiv:2101.07364v3 [astro-ph.IM] UPDATED)
› Stellar Evolution and Tidal Dissipation in REBOUNDx. (arXiv:2101.12277v2 [astro-ph.SR] UPDATED)
› The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations. (arXiv:2102.13603v2 [astro-ph.GA] UPDATED)
› Forward Modelling the O3(a+b) GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions. (arXiv:2105.05783v4 [astro-ph.HE] UPDATED)
› Testing the Kerr black hole hypothesis with GRS 1716-249 by combining the continuum-fitting and the iron-line methods. (arXiv:2106.03086v2 [astro-ph.HE] UPDATED)
› Wide-field X-ray observations of the supernova remnant Puppis A with the SRG/ART-XC telescope. (arXiv:2107.05586v2 [astro-ph.HE] UPDATED)
› A full spectral-timing model to map the accretion flow in black hole binaries: the low/hard state of MAXI J1820+070. (arXiv:2107.12517v3 [astro-ph.HE] UPDATED)
› Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations. (arXiv:2107.13168v2 [astro-ph.GA] UPDATED)
› Cosmic ray Transport in Magnetohydrodynamic turbulence. (arXiv:2108.01936v2 [astro-ph.HE] UPDATED)
› Time Delay Interferometry combinations as instrument noise monitors for LISA. (arXiv:2108.02738v3 [gr-qc] UPDATED)
› LkH$\alpha$ 225 (V1318 Cyg) South in Outburst. (arXiv:2108.05406v2 [astro-ph.SR] UPDATED)
› Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters. (arXiv:2108.06790v2 [astro-ph.CO] UPDATED)
› Josephson junction formed in the wormhole space time from the analysis for the critical temperature of BEC. (arXiv:2108.08030v2 [hep-th] UPDATED)
› Effects of Small-Scale Absorption Systems on Neutral Islands during the Late Epoch of Reionization. (arXiv:2108.10229v2 [astro-ph.CO] UPDATED)
› The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis \`a vis One-Dimensional, Massive-star Supernova Progenitor Models. (arXiv:2109.10920v3 [astro-ph.SR] UPDATED)
› Gravitational Collapse in the Post-Inflationary Universe. (arXiv:2110.15109v2 [astro-ph.CO] UPDATED)
› Multi-wavelength emission from leptonic processes in ageing galaxy bubbles. (arXiv:2111.00204v2 [astro-ph.HE] UPDATED)
› INTEGRAL/IBIS 17-yr hard X-ray all-sky survey. (arXiv:2111.02996v2 [astro-ph.HE] UPDATED)
› Exploring Gravitationally-Lensed $z\gtrsim6$ X-ray AGN Behind the RELICS clusters. (arXiv:2111.03669v2 [astro-ph.GA] UPDATED)
› On the origin and the detection of characteristic axion wiggles in photon spectra. (arXiv:2111.08303v2 [astro-ph.HE] UPDATED)
› Effective actions for compact objects in an effective field theory of gravity. (arXiv:2111.09070v3 [hep-th] UPDATED)
› PBH formation from spherically symmetric hydrodynamical perturbations: a review. (arXiv:2111.12693v2 [gr-qc] UPDATED)
› How the Galaxy Stellar Spins Acquire a Peculiar Tidal Connection?. (arXiv:2111.13831v2 [astro-ph.GA] UPDATED)
› The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data. (arXiv:2112.02026v2 [astro-ph.GA] UPDATED)
› A Faster Growth of Perturbations in an Early Matter Dominated Epoch: Primordial Black Holes and Gravitational Waves. (arXiv:2112.11486v2 [astro-ph.CO] UPDATED)
› Sound velocity effects on the phase transition gravitational wave spectrum in the Sound Shell Model. (arXiv:2112.14650v2 [astro-ph.CO] UPDATED)
› Revisiting the constraints on primordial black hole abundance with the isotropic gamma ray background. (arXiv:2112.15463v2 [astro-ph.CO] UPDATED)
› Hydrothermal activities on C-complex asteroids induced by radioactivity. (arXiv:2201.00996v2 [astro-ph.EP] UPDATED)
› Detailed analysis on the reflection component for the black hole candidate MAXI J1348-630. (arXiv:2201.01207v2 [astro-ph.HE] UPDATED)
› Improved bounds on ultralight scalar dark matter in the radio-frequency range. (arXiv:2201.02042v2 [hep-ph] UPDATED)
› Haro 11 -- Untying the knots of the nuclear starburst. (arXiv:2201.03585v2 [astro-ph.GA] UPDATED)
› Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white-dwarfs. (arXiv:2201.03827v2 [astro-ph.SR] UPDATED)
› Multiparticle collision simulations of dense stellar systems and plasmas. (arXiv:2201.04586v2 [astro-ph.GA] UPDATED)
› The Large High Altitude Air Shower Observatory (LHAASO) Science White Paper -- 2021 Edition. (arXiv:1905.02773v2 [astro-ph.HE] CROSS LISTED)

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