Spectral Methods for Numerical Relativity
... Einstein’s equations represent a complicated set of nonlinear partial differential equations for which some exact [30] or approximate [31] analytical solutions are known. But these solutions are not always suitable for physically or astrophysically interesting systems, which require an accurate desc ...
... Einstein’s equations represent a complicated set of nonlinear partial differential equations for which some exact [30] or approximate [31] analytical solutions are known. But these solutions are not always suitable for physically or astrophysically interesting systems, which require an accurate desc ...
sdssv13 - Sloan Digital Sky Survey
... How much dark matter is there? Local census of the galaxy population: How did galaxies form? Find the most distant objects in the Universe: What are the highest quasar redshifts? ...
... How much dark matter is there? Local census of the galaxy population: How did galaxies form? Find the most distant objects in the Universe: What are the highest quasar redshifts? ...
Session 1: Stellar winds, diagnostics across the electromagnetic
... across the full range of wavelengths, polarimetry provides a window into a variety of stellar phenomena not accessible by other means. For example, polarimetry constrains the properties of circumstellar disks, unveils details of the magnetic fields in molecular cloud cores, and reveals the complex g ...
... across the full range of wavelengths, polarimetry provides a window into a variety of stellar phenomena not accessible by other means. For example, polarimetry constrains the properties of circumstellar disks, unveils details of the magnetic fields in molecular cloud cores, and reveals the complex g ...
Diffraction-Based Sensitivity Analysis of Apodized Pupil Mapping Systems
... Pluzhnik et al. (2006), a hybrid pupil mapping system was proposed that combines the pupil mapping mirrors with a modest apodization of oversized entrance and exit pupils. This combination does indeed achieve the needed high-contrast point spread function (PSF). In this paper, we call such systems a ...
... Pluzhnik et al. (2006), a hybrid pupil mapping system was proposed that combines the pupil mapping mirrors with a modest apodization of oversized entrance and exit pupils. This combination does indeed achieve the needed high-contrast point spread function (PSF). In this paper, we call such systems a ...
Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies
... luminous galaxies form and initially evolve as disk galaxies at the center of isolated dark matter halos (DMH). Under this paradigm, as dark matter over-densities decouple from the large scale flow and collapse, the baryons of the ambient intergalactic medium bound to the potential well of the nasce ...
... luminous galaxies form and initially evolve as disk galaxies at the center of isolated dark matter halos (DMH). Under this paradigm, as dark matter over-densities decouple from the large scale flow and collapse, the baryons of the ambient intergalactic medium bound to the potential well of the nasce ...
TMT Science Overview - GSMT Program Office
... The authors gratefully acknowledge the support of the TMT partner institutions. They are the Association of Canadian Universities for Research in Astronomy (ACURA), the Association of Universities for Research in Astronomy (AURA), the California Institute of Technology and the University of Californ ...
... The authors gratefully acknowledge the support of the TMT partner institutions. They are the Association of Canadian Universities for Research in Astronomy (ACURA), the Association of Universities for Research in Astronomy (AURA), the California Institute of Technology and the University of Californ ...
Gravitational-wave signal from binary neutron star merger
... the post-merger phase, where numerical relativity is the only available investigation tool. For the models which form an hyper-massive neutron star after the merger, the impact of different source parameters on the post-merger spectrum and radiated energy is analysed (sec. 4.2.1), including the role ...
... the post-merger phase, where numerical relativity is the only available investigation tool. For the models which form an hyper-massive neutron star after the merger, the impact of different source parameters on the post-merger spectrum and radiated energy is analysed (sec. 4.2.1), including the role ...
YEAR - University of Maryland Astronomy
... Chesire Cats and Black Holes Defining Pluto: Planet or hunk of unplanetlike rock? Searching for Life in the Universe The Sun's Magnificent Magnetic Field Monsters in the Sky: Quasars and Supermassive Black Holes Gas in Galaxies Mysteries in the Heart of Galaxies Formation of Planetary Systems Faster ...
... Chesire Cats and Black Holes Defining Pluto: Planet or hunk of unplanetlike rock? Searching for Life in the Universe The Sun's Magnificent Magnetic Field Monsters in the Sky: Quasars and Supermassive Black Holes Gas in Galaxies Mysteries in the Heart of Galaxies Formation of Planetary Systems Faster ...
Galaxy Evolution Over the Past Eleven Billion Years: Mergers and
... Galaxy evolution studies have been revolutionized by the advent of near-infrared observations over the last decade. An intriguingly population of distant red galaxies, only visible at near-infrared wavelengths, was discovered. They were previously overlooked, since they are invisible even in the dee ...
... Galaxy evolution studies have been revolutionized by the advent of near-infrared observations over the last decade. An intriguingly population of distant red galaxies, only visible at near-infrared wavelengths, was discovered. They were previously overlooked, since they are invisible even in the dee ...
