Search Results - "POGOSYAN, D"
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SPECTRUM AND ANISOTROPY OF TURBULENCE FROM MULTI-FREQUENCY MEASUREMENT OF SYNCHROTRON POLARIZATION
Published in The Astrophysical journal (20-02-2016)“…ABSTRACT We consider turbulent synchrotron-emitting media that also exhibit Faraday rotation and provide a statistical description of synchrotron polarization…”
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STATISTICAL DESCRIPTION OF SYNCHROTRON INTENSITY FLUCTUATIONS: STUDIES OF ASTROPHYSICAL MAGNETIC TURBULENCE
Published in The Astrophysical journal (01-03-2012)“…We provide a theoretical description of synchrotron fluctuations arising from magnetic turbulence. We derive an expression that relates the correlation of…”
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Extending velocity channel analysis for studying turbulence anisotropies
Published in Monthly notices of the Royal Astronomical Society (11-09-2016)“…We extend the velocity channel analysis (VCA), introduced by Lazarian & Pogosyan, of the intensity fluctuations in the velocity slices of…”
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Galaxy evolution in the metric of the cosmic web
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract The role of the cosmic web in shaping galaxy properties is investigated in the Galaxy And Mass Assembly (GAMA) spectroscopic survey in the redshift…”
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Study of velocity centroids based on the theory of fluctuations in position–position–velocity space
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…We study the possibility of obtaining power spectrum of gas velocity in the turbulent interstellar medium from spatial correlation of velocity centroids (VCs)…”
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Dancing in the dark: galactic properties trace spin swings along the cosmic web
Published in Monthly notices of the Royal Astronomical Society (21-10-2014)“…A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments…”
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Swirling around filaments: are large-scale structure vortices spinning up dark haloes?
Published in Monthly notices of the Royal Astronomical Society (21-01-2015)“…The kinematic analysis of dark matter and hydrodynamical simulations suggests that the vorticity in large-scale structure is mostly confined to, and…”
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Nature of striation in 21 cm channel Maps: velocity caustics
Published in Monthly notices of the Royal Astronomical Society (12-07-2023)“…ABSTRACT The alignment of striated intensity structures in thin neutral hydrogen (H i) spectroscopic channels with Galactic magnetic fields has been observed…”
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Statistical properties of Galactic CMB foregrounds: dust and synchrotron
Published in Monthly notices of the Royal Astronomical Society (21-07-2018)“…ABSTRACT Recent Planck observations have revealed some of the important statistical properties of synchrotron and dust polarization, namely, the B to E mode…”
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Rigging dark haloes: why is hierarchical galaxy formation consistent with the inside-out build-up of thin discs?
Published in Monthly notices of the Royal Astronomical Society (01-12-2011)“…State-of-the-art hydrodynamical simulations show that gas inflow through the virial sphere of dark matter haloes is focused (i.e. has a preferred inflow…”
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Non-Gaussian Minkowski functionals and extrema counts in redshift space
Published in Monthly notices of the Royal Astronomical Society (11-10-2013)“…In the context of upcoming large-scale structure surveys such as Euclid, it is of prime importance to quantify the effect of peculiar velocities on geometric…”
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The clustering of critical points in the evolving cosmic web
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT Focusing on both small separations and baryonic acoustic oscillation scales, the cosmic evolution of the clustering properties of peak, void, wall,…”
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Intrinsic alignment of simulated galaxies in the cosmic web: implications for weak lensing surveys
Published in Monthly notices of the Royal Astronomical Society (21-04-2015)“…The intrinsic alignment of galaxy shapes (by means of their angular momentum) and their cross-correlation with the surrounding dark matter tidal field are…”
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Non-Gaussianity and Minkowski functionals: forecasts for Planck
Published in Monthly notices of the Royal Astronomical Society (01-03-2013)“…We study Minkowski functionals as probes of primordial non-Gaussianity in the cosmic microwave background, specifically for the estimate of the primordial…”
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Connecting the cosmic web to the spin of dark haloes: implications for galaxy formation
Published in Monthly notices of the Royal Astronomical Society (21-12-2012)“…ABSTRACT We investigate the alignment of the spin of dark matter haloes relative (i) to the surrounding large‐scale filamentary structure, and (ii) to the…”
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STUDYING THE INTERSTELLAR MAGNETIC FIELD FROM ANISOTROPIES IN VELOCITY CHANNELS
Published in The Astrophysical journal (20-11-2015)“…ABSTRACT Turbulence in the interstellar medium is anisotropic due to the ubiquitous magnetic fields. This anisotropy depends on the strength of the magnetic…”
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When do cosmic peaks, filaments, or walls merge? A theory of critical events in a multiscale landscape
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT The merging rate of cosmic structures is computed, relying on the ansatz that they can be predicted in the initial linear density field from the…”
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Studying Turbulence Using Doppler-broadened Lines: Velocity Coordinate Spectrum
Published in The Astrophysical journal (01-12-2006)“…We discuss a new technique for studying astrophysical turbulence that utilizes the statistics of Doppler-broadened spectral lines. The technique relates the…”
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Velocity Modification of the Power Spectrum from an Absorbing Medium
Published in The Astrophysical journal (01-12-2004)“…A quantitative description of the statistics of intensity fluctuations within spectral line data cubes introduced in our earlier work is extended to the…”
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Studying Velocity Turbulence from Doppler-broadened Absorption Lines: Statistics of Optical Depth Fluctuations
Published in The Astrophysical journal (10-10-2008)“…We continue our work on developing techniques for studying turbulence with spectroscopic data. We show that Doppler-broadened absorption spectral lines, in…”
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