Najnowsze prace na astro-ph:

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› The gas fractions of dark matter haloes hosting simulated $\sim L^\star$ galaxies are governed by the feedback history of their black holes. (arXiv:1810.07696v1 [astro-ph.GA])
› Complete ejection of OB stars from very young star clusters and the formation of multiple populations. (arXiv:1810.07697v1 [astro-ph.SR])
› UV background fluctuations traced by metal ions at $z\approx3$. (arXiv:1810.07699v1 [astro-ph.GA])
› Circumgalactic gas at its extreme: tidal gas streams around the Whale galaxy NGC 4631 explored with HST/COS. (arXiv:1810.07700v1 [astro-ph.GA])
› Barred galaxies in cosmological zoom-in simulations: the importance of feedback. (arXiv:1810.07701v1 [astro-ph.GA])
› Radii of 88 M Subdwarfs and Updated Radius Relations for Low-Metallicity M Dwarf Stars. (arXiv:1810.07702v1 [astro-ph.SR])
› A Deep Learning Approach to Galaxy Cluster X-ray Masses. (arXiv:1810.07703v1 [astro-ph.CO])
› Reverse Direct Detection: Cosmic Ray Scattering With Light Dark Matter. (arXiv:1810.07705v1 [hep-ph])
› Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory. (arXiv:1810.07707v1 [astro-ph.GA])
› On the Diagnostic Power of FIR/Sub-mm SED Fitting in Massive Galactic Molecular Clumps. (arXiv:1810.07708v1 [astro-ph.GA])
› Logarithmic-corrected $R^2$ Gravity Inflation in the Presence of Kalb-Ramond Fields. (arXiv:1810.07711v1 [gr-qc])
› Alfv\'en Wave Dissipation in the Solar Chromosphere. (arXiv:1810.07712v1 [astro-ph.SR])
› The evolution of the warm absorber reveals a shocked outflow in the narrow line Seyfert 1 galaxy IRAS 17020+4544. (arXiv:1810.07714v1 [astro-ph.GA])
› Explaining the asymmetric line profile in Cepheus X-4 with spectral variation across pulse phase. (arXiv:1810.07724v1 [astro-ph.HE])
› Resonance-broadened transit time damping of particles in MHD turbulence. (arXiv:1810.07726v1 [astro-ph.HE])
› The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation. (arXiv:1810.07727v1 [astro-ph.CO])
› Configuration entropy in the $\Lambda$CDM and the dynamical dark energy models: Can we distinguish one from the other?. (arXiv:1810.07729v1 [astro-ph.CO])
› Signature of a Cosmic String Wake at $z=5$. (arXiv:1810.07737v1 [astro-ph.CO])
› Simultaneous VLBI Astrometry of H2O and SiO Masers toward the Semiregular Variable R Crateris. (arXiv:1810.07739v1 [astro-ph.SR])
› The $^{12}$CO$_2$ and $^{13}$CO$_2$ Absorption Bands as Tracers of the Thermal History of Interstellar Icy Grain Mantles. (arXiv:1810.07754v1 [astro-ph.IM])
› The origin of galactic metal-rich stellar halo components with highly eccentric orbits. (arXiv:1810.07779v1 [astro-ph.GA])
› Return to the Kuiper Belt: launch opportunities from 2025 to 2040. (arXiv:1810.07811v1 [astro-ph.EP])
› Luminosity and cooling suppression in magnetized white dwarfs. (arXiv:1810.07836v1 [astro-ph.SR])
› Metals, depletion and dimming: decrypting dust. (arXiv:1810.07843v1 [astro-ph.GA])
› Multiband galaxy morphologies for CLASH: a convolutional neural network transferred from CANDELS. (arXiv:1810.07857v1 [astro-ph.IM])
› Stiff Matter Solution in Brans-Dicke Theory and The General Relativity Limit. (arXiv:1810.07860v1 [gr-qc])
› Science with an ngVLA: High-resolution imaging of comets. (arXiv:1810.07867v1 [astro-ph.EP])
› Populations of accreting white dwarfs. (arXiv:1810.07878v1 [astro-ph.SR])
› Classifying Lensed Gravitational Waves in the Geometrical Optics Limit with Machine Learning. (arXiv:1810.07888v1 [astro-ph.IM])
› Astrospheres and Cosmic Rays. (arXiv:1810.07940v1 [astro-ph.SR])
› Pebble trapping backreaction does not destroy vortices. (arXiv:1810.07941v1 [astro-ph.EP])
› Dispersive shock waves in partially ionised plasmas. (arXiv:1810.07948v1 [astro-ph.SR])
› Most general cubic-order Horndeski Lagrangian allowing for scaling solutions and the application to dark energy. (arXiv:1810.07957v1 [gr-qc])
› Remodeling the evolution of grain size distribution in galaxies. (arXiv:1810.07962v1 [astro-ph.GA])
› What sets the magnetic field strength and cycle period in solar-type stars?. (arXiv:1810.07978v1 [astro-ph.SR])
› Temperature-dependent oscillation modes in rotating superfluid neutron stars. (arXiv:1810.08005v1 [astro-ph.HE])
› Characterisation of the radial oxygen abundance distribution in disk galaxies. (arXiv:1810.08006v1 [astro-ph.GA])
› Spectral analysis of magnetic fields in simulated galaxy clusters. (arXiv:1810.08009v1 [astro-ph.CO])
› Intensity Interferometry revival on the C\^ote d'Azur. (arXiv:1810.08023v1 [astro-ph.IM])
› CME-driven shock and Type II solar radio burst band-splitting. (arXiv:1810.08026v1 [astro-ph.SR])
› Multi Photon Absorption in Gravity Induced Resonant Emission. (arXiv:1810.08041v1 [physics.plasm-ph])
› A new method to derive star formation histories in dwarf galaxies. (arXiv:1810.08045v1 [astro-ph.GA])
› A quantitative NLTE analysis of visual and ultraviolet spectra of four helium-rich subdwarf O stars. (arXiv:1810.08082v1 [astro-ph.SR])
› Parameter discordance in Planck CMB and low-redshift measurements: projection in the primordial power spectrum. (arXiv:1810.08101v1 [astro-ph.CO])
› SWEET-Cat updated. New homogenous spectroscopic parameters. (arXiv:1810.08108v1 [astro-ph.EP])
› High-redshift radio galaxies at low radio frequencies. (arXiv:1810.08119v1 [astro-ph.GA])
› RELICS: High-Resolution Constraints on the Inner Mass Distribution of the z=0.83 Merging Cluster RXJ0152.7-1357 from strong lensing. (arXiv:1810.08122v1 [astro-ph.CO])
› Towards purely geometric inflation and late time acceleration. (arXiv:1810.08166v1 [gr-qc])
› The physics of Lyman-alpha escape from high-redshift galaxies. (arXiv:1810.08185v1 [astro-ph.GA])
› Science with an ngVLA: The ngVLA Reference Design. (arXiv:1810.08197v1 [astro-ph.IM])
› Heating up the Galaxy with Hidden Photons. (arXiv:1509.00039v2 [hep-ph] UPDATED)
› Towards de Sitter from 10D. (arXiv:1707.08678v2 [hep-th] UPDATED)
› Dynamical effects in the observed rate of change of the orbital and the spin periods of radio pulsars: Improvement in the method of estimation and its implications. (arXiv:1712.06590v2 [astro-ph.IM] UPDATED)
› Muon Radiation Dose and Marine Megafaunal Extinction at the end-Pliocene Supernova. (arXiv:1712.09367v2 [astro-ph.EP] UPDATED)
› The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights. (arXiv:1801.03043v3 [astro-ph.CO] UPDATED)
› The massive Dirac equation in the curved spacetime of the Kerr-Newman (anti) de Sitter black hole. (arXiv:1801.03157v3 [gr-qc] UPDATED)
› Scaling Relations for Dark Matter Annihilation and Decay Profiles in Dwarf Spheroidal Galaxies. (arXiv:1802.06811v2 [astro-ph.GA] UPDATED)
› Multi-messenger constraints to the local emission of cosmic-ray electrons. (arXiv:1803.01009v2 [astro-ph.HE] UPDATED)
› Characterizing optical variability of OJ 287 in 2016 - 2017. (arXiv:1803.03964v2 [astro-ph.HE] UPDATED)
› Search for neutrinos from decaying dark matter with IceCube. (arXiv:1804.03848v2 [astro-ph.HE] UPDATED)
› Black Hole Mergers From Globular Clusters Observable by LISA II: Resolved Eccentric Sources and the Gravitational Wave Background. (arXiv:1805.06194v2 [astro-ph.HE] UPDATED)
› Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations. (arXiv:1805.09371v2 [astro-ph.HE] UPDATED)
› Nuclear processes in Astrophysics: Recent progress. (arXiv:1805.10183v2 [astro-ph.SR] UPDATED)
› Density Waves and the Viscous Overstability in Saturn's Rings. (arXiv:1806.01211v3 [astro-ph.EP] UPDATED)
› Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics. (arXiv:1806.11118v2 [astro-ph.GA] UPDATED)
› Revealing Dusty Supernovae in High-Redshift (Ultra-)Luminous InfraRed Galaxies Through Near-Infrared Integrated Light Variability. (arXiv:1808.01780v2 [astro-ph.GA] UPDATED)
› Nearby high-speed stars in Gaia DR2. (arXiv:1808.02620v2 [astro-ph.GA] UPDATED)
› Analytical estimates of proton acceleration in laser-produced turbulent plasmas. (arXiv:1808.04356v2 [astro-ph.HE] UPDATED)
› Climates of Warm Earth-like Planets I: 3-D Model Simulations. (arXiv:1808.06480v2 [astro-ph.EP] UPDATED)
› ASASSN-18ey: The Rise of a New Black-Hole X-ray Binary. (arXiv:1808.07875v2 [astro-ph.HE] UPDATED)
› Science with an ngVLA: Dust growth and dust trapping in protoplanetary disks. (arXiv:1809.06403v2 [astro-ph.EP] UPDATED)
› Rapidly-evolving episodic outflow in IRAS 18113-2503: clues to the ejection mechanism of the fastest water fountain. (arXiv:1809.07505v2 [astro-ph.SR] UPDATED)
› Steep Eternal Inflation and the Swampland. (arXiv:1810.03438v2 [gr-qc] UPDATED)
› First high-resolution look at the quiet Sun with ALMA at 3 mm. (arXiv:1810.05223v2 [astro-ph.SR] UPDATED)
› Opening the energy window on direct dark matter detection. (arXiv:1810.05576v2 [hep-ph] UPDATED)
› Quintessential Starobinsky inflation and swampland criteria. (arXiv:1810.06445v2 [hep-th] UPDATED)
› Cosmic Ray Extremely Distributed Observatory: a global network of detectors to probe contemporary physics mysteries. (arXiv:1810.06953v3 [astro-ph.IM] UPDATED)
› The MOSDEF Survey: Stellar Continuum Spectra and Star Formation Histories of Active, Transitional, and Quiescent Galaxies at 1.4$
› An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S. (arXiv:1810.07445v2 [astro-ph.GA] UPDATED)
› Inflation with $R^2$ term in the Palatini formalism. (arXiv:1810.05536v1 [gr-qc] CROSS LISTED)
› Flavor structures in the Dark Standard Model TeV-Paradigm. (arXiv:1810.07198v1 [hep-ph] CROSS LISTED)
› Gravitational Lenses as High-Resolution Telescopes. (arXiv:1810.07265v1 [astro-ph.HE] CROSS LISTED)

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