Najnowsze prace na astro-ph:

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› Empirically determined dilution factors of stripped-envelope, core-collapse SNe: Paper II - Using GRB-SNe to determine the Hubble Constant. (arXiv:1805.06892v1 [astro-ph.CO])
› Kinematics of outer halo globular clusters: M 75 and NGC 6426. (arXiv:1805.06894v1 [astro-ph.GA])
› The Formation of Ultra Diffuse Galaxies in Cored Dark Matter Halos Through Tidal Stripping and Heating. (arXiv:1805.06896v1 [astro-ph.GA])
› SNe Kicks in Hierarchical Triple Systems. (arXiv:1805.06897v1 [astro-ph.SR])
› Gas-Assisted Growth of Protoplanets in a Turbulent Medium. (arXiv:1805.06898v1 [astro-ph.EP])
› Gravitational Wave Signals from the First Massive Black Hole Seeds. (arXiv:1805.06901v1 [astro-ph.GA])
› Cosmological simulations of black hole growth II: how (in)significant are merger events for fuelling nuclear activity?. (arXiv:1805.06902v1 [astro-ph.GA])
› A Theory for the Variation of Dust Attenuation Laws in Galaxies. (arXiv:1805.06905v1 [astro-ph.GA])
› Type Ia supernovae have two physical width-luminosity relations and they favor sub-Chandrasekhar and direct collision models - II. Color evolution. (arXiv:1805.06907v1 [astro-ph.HE])
› Spectroscopic decomposition of the galaxy and halo of the cD galaxy NGC 3311. (arXiv:1805.06913v1 [astro-ph.GA])
› Morphology of AGN Emission Line Regions in SDSS-IV MaNGA Survey. (arXiv:1805.06916v1 [astro-ph.GA])
› C/2016 R2 (PANSTARRS): A comet rich in CO and depleted in HCN. (arXiv:1805.06918v1 [astro-ph.EP])
› A Mid-IR Selected Changing-Look Quasar and Physical Scenarios for Abrupt AGN Fading. (arXiv:1805.06920v1 [astro-ph.GA])
› A new physical interpretation of optical and infrared variability in quasars. (arXiv:1805.06921v1 [astro-ph.GA])
› Preparing the NIRSpec/JWST science data calibration: from ground testing to sky. (arXiv:1805.06922v1 [astro-ph.IM])
› TDEM final report: Enhanced direct imaging exoplanet detection with astrometry mass determination. (arXiv:1805.06933v1 [astro-ph.IM])
› The case for a cold dark matter cusp in Draco. (arXiv:1805.06934v1 [astro-ph.GA])
› The impact of assembly bias on the halo occupation in hydrodynamical simulations. (arXiv:1805.06938v1 [astro-ph.GA])
› Scientific Discovery with the James Webb Space Telescope. (arXiv:1805.06941v1 [astro-ph.IM])
› Long Term Planetary Habitability and the Carbonate-Silicate Cycle. (arXiv:1805.06943v1 [astro-ph.EP])
› Signatures of the disk-jet coupling in the Broad-line Radio Quasar 4C+74.26. (arXiv:1805.06957v1 [astro-ph.HE])
› Luminous WISE-selected Obscured, Unobscured, and Red Quasars in Stripe 82. (arXiv:1805.06961v1 [astro-ph.GA])
› Winds of Massive Stars: High Resolution X-ray Spectra of Stars in NGC 3603. (arXiv:1805.06973v1 [astro-ph.SR])
› On the Nature of Long-Period Dwarf Novae with Rare and Low-Amplitude Outbursts. (arXiv:1805.06974v1 [astro-ph.SR])
› Cosmological cluster tension. (arXiv:1805.06976v1 [astro-ph.CO])
› Peer-review under review - A statistical study on proposal ranking at ESO. Part I: the pre-meeting phase. (arXiv:1805.06981v1 [physics.soc-ph])
› Forward modelling of quasar light curves and the cosmological matter power spectrum on milliparsec scales. (arXiv:1805.06984v1 [astro-ph.CO])
› Exploring possible relations between optical variability time scales and broad emission line shapes in AGN. (arXiv:1805.07007v1 [astro-ph.GA])
› VLT/X-shooter GRBs: Individual extinction curves of star-forming regions. (arXiv:1805.07016v1 [astro-ph.GA])
› The growth of stellar mass black hole binaries trapped in an accretion disk of active galactic nuclei. (arXiv:1805.07026v1 [astro-ph.HE])
› Solar cycle observations of the Neon abundance in the Sun-as-a-star. (arXiv:1805.07032v1 [astro-ph.SR])
› Reliability of stellar inclination estimated from asteroseismology: analytical criteria, mock simulations and Kepler data analysis. (arXiv:1805.07044v1 [astro-ph.SR])
› The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation. (arXiv:1805.07062v1 [astro-ph.GA])
› Discovery of deep eclipses in the cataclysmic variable IPHAS J051814.33+294113.0. (arXiv:1805.07065v1 [astro-ph.SR])
› Which evolutionary status does the Blue Large-Amplitude Pulsators stay at?. (arXiv:1805.07073v1 [astro-ph.SR])
› The Gaia-ESO Survey: properties of newly discovered Li-rich giants. (arXiv:1805.07077v1 [astro-ph.SR])
› The Excess Density of Field Galaxies near z=0.56 around the Gamma-Ray Burst GRB021004 Position. (arXiv:1805.07082v1 [astro-ph.GA])
› Automatic vetting of planet candidates from ground based surveys: Machine learning with NGTS. (arXiv:1805.07089v1 [astro-ph.EP])
› Impact degassing and atmospheric erosion on Venus, Earth, and Mars during the late accretion. (arXiv:1805.07094v1 [astro-ph.EP])
› KIC 3240411 - the hottest known SPB star with the asymptotic g-mode period spacing. (arXiv:1805.07100v1 [astro-ph.SR])
› A new universal cosmic-ray knee near the magnetic rigidity 10 TV with the NUCLEON space observatory. (arXiv:1805.07119v1 [astro-ph.HE])
› Time-dependent Pattern Speeds in Barred Galaxies. (arXiv:1805.07131v1 [astro-ph.GA])
› Kinetic Sunyaev--Zel'dovich effect in rotating galaxy clusters from MUSIC simulations. (arXiv:1805.07142v1 [astro-ph.CO])
› A new parametrization of dark energy equation of state leading to double exponential potential. (arXiv:1805.07148v1 [gr-qc])
› Bayesian optimisation for likelihood-free cosmological inference. (arXiv:1805.07152v1 [astro-ph.CO])
› Hubble Tarantula Treasury Project - VI. Identification of Pre-Main-Sequence Stars using Machine Learning techniques. (arXiv:1805.07157v1 [astro-ph.SR])
› New classification of solar flares based on the maximum flux in Soft X-rays and on duration of flare. (arXiv:1805.07158v1 [astro-ph.SR])
› Planets, candidates, and binaries from the CoRoT/Exoplanet programme: the CoRoT transit catalogue. (arXiv:1805.07164v1 [astro-ph.EP])
› The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter. (arXiv:1805.07165v1 [astro-ph.GA])
› Multivariate analysis of cosmic void characteristics. (arXiv:1805.07181v1 [astro-ph.CO])
› Dynamical and observational constraints on the Warm Little Inflaton scenario. (arXiv:1805.07186v1 [astro-ph.CO])
› Magnetic Field Saturation of the Ion Weibel Instability in Interpenetrating Relativistic Plasmas. (arXiv:1805.07188v1 [astro-ph.HE])
› Spatially Resolved Metal Gas Clouds. (arXiv:1805.07192v1 [astro-ph.GA])
› The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136. (arXiv:1805.07212v1 [astro-ph.GA])
› The Kinetic Theory of the Mesoscopic Spacetime. (arXiv:1805.07218v1 [gr-qc])
› Molecular Cloud Evolution VI. Measuring cloud ages. (arXiv:1805.07221v1 [astro-ph.GA])
› The Star Formation History in the M31 Bulge. (arXiv:1805.07225v1 [astro-ph.GA])
› Global-scale equatorial Rossby waves as an essential component of solar internal dynamics. (arXiv:1805.07244v1 [astro-ph.SR])
› ELT-scale Adaptive Optics real-time control with thes Intel Xeon Phi Many Integrated Core Architecture. (arXiv:1805.07254v1 [astro-ph.IM])
› White dwarfs with a surface electrical charge distribution: Equilibrium and stability. (arXiv:1805.07257v1 [astro-ph.SR])
› Models for Type Ia supernovae and related astrophysical transients. (arXiv:1805.07268v1 [astro-ph.SR])
› The Effect of Minimum Length and Maximum Length in Cosmology. (arXiv:1805.07278v1 [astro-ph.CO])
› Multifractality Signatures in Quasars Time Series. I. 3C 273. (arXiv:1805.07287v1 [astro-ph.GA])
› Cloud-Cloud Collision Induced Star Formation in IRAS 18223-1243. (arXiv:1805.07305v1 [astro-ph.GA])
› The fraction of ionizing radiation from massive stars that escapes to the intergalactic medium. (arXiv:1805.07318v1 [astro-ph.GA])
› Ground-based optical transmission spectroscopy of the small, rocky exoplanet GJ 1132b. (arXiv:1805.07328v1 [astro-ph.EP])
› Gravitino Decay in High Scale Supersymmetry with R-parity Violation. (arXiv:1805.07342v1 [hep-ph])
› Organic chemistry in a CO2 rich early Earth atmosphere. (arXiv:1805.07347v1 [astro-ph.EP])
› Saving Early Disk Formation of Young Stellar Objects from the Magnetic Braking Catastrophe. (arXiv:1805.07348v1 [astro-ph.SR])
› A Gaia DR~2 and VLT/FLAMES search for new satellites of the LMC. (arXiv:1805.07350v1 [astro-ph.GA])
› Quantitative Spectroscopy of Supergiants in the Local Group Dwarf Galaxy IC 1613: Metallicity and Distance. (arXiv:1805.07352v1 [astro-ph.GA])
› Large-scale structure in mimetic Horndeski gravity. (arXiv:1708.01850v2 [astro-ph.CO] UPDATED)
› Cross section alignment of polycyclic aromatic hydrocarbons by anisotropic radiation. (arXiv:1710.01835v2 [astro-ph.GA] UPDATED)
› A cocoon shock breakout as the origin of the $ \gamma $-ray emission in GW170817. (arXiv:1710.05896v2 [astro-ph.HE] UPDATED)
› Radiative cooling of swept up gas in AGN-driven galactic winds and its implications for molecular outflows. (arXiv:1710.09433v2 [astro-ph.GA] UPDATED)
› On the radial acceleration relation of $\Lambda$CDM satellite galaxies. (arXiv:1712.04448v2 [astro-ph.GA] UPDATED)
› Gravitational probes of dark matter physics. (arXiv:1712.06615v2 [astro-ph.CO] UPDATED)
› Century of $\Lambda$. (arXiv:1712.09845v3 [physics.hist-ph] UPDATED)
› Scalaron from $R^2$-gravity as a Heavy Field. (arXiv:1712.09896v2 [astro-ph.CO] UPDATED)
› Measuring oxygen abundances from stellar spectra without oxygen lines. (arXiv:1801.07370v2 [astro-ph.SR] UPDATED)
› ALMA 26 Arcmin$^{2}$ Survey of GOODS-S at One-millimeter (ASAGAO): Average Morphology of High-$z$ Dusty Star-Forming Galaxies is an Exponential-Disk ($n \simeq 1$). (arXiv:1802.02136v2 [astro-ph.GA] UPDATED)
› About 30% of Sun-like Stars Have Kepler-like Planetary Systems: A Study of their Intrinsic Architecture. (arXiv:1802.09526v2 [astro-ph.EP] UPDATED)
› First predictions of the angular power spectrum of the astrophysical gravitational wave background. (arXiv:1803.03236v2 [astro-ph.CO] UPDATED)
› Parametrizing the Reionization History with the Redshift Midpoint, Duration, and Asymmetry. (arXiv:1804.00672v2 [astro-ph.CO] UPDATED)
› Constraining the Polarization Content of Gravitational Waves with Astrometry. (arXiv:1804.03146v2 [gr-qc] UPDATED)
› EDGES result versus CMB and low-redshift constraints on ionization histories. (arXiv:1804.03888v2 [astro-ph.CO] UPDATED)
› Monitoring near-Earth-object discoveries for imminent impactors. (arXiv:1805.01315v3 [astro-ph.EP] UPDATED)
› Parallactic distances and proper motions of virtually all stars in the sigma Orionis cluster or: How I learned to get the most out of TOPCAT and love Gaia DR2. (arXiv:1805.05092v2 [astro-ph.SR] UPDATED)
› Ghost Free Mimetic Massive Gravity. (arXiv:1805.06283v2 [hep-th] UPDATED)
› 15-GHz radio emission from nearby low-luminosity active galactic nuclei. (arXiv:1805.06696v2 [astro-ph.HE] UPDATED)

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