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Standing in Awe - Auckland Astronomical Society
Standing in Awe - Auckland Astronomical Society

... Libra lies prominently in the June sky, preceding the Scorpion across the sky. At 538° square in size, Libra is one of the larger constellations, though its stars are poorly shown, the brightest attaining magnitude 2.6. In fact, Libra is one of the poorer adorned constellations, there being only 2.4 ...
Spiral galaxies: Spiral galaxies: Inclination Spiral galaxies: Internal
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... – Since the amount of visible matter is declining exponentially, the mass must be coming from a “dark halo” that extends out to ~100 – 200 kpc – Since there is no visible matter to see, it is hard to measure total masses of spirals! – What does this imply for the density profile of the dark halo? To ...
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... should electrostatically explode in vacuum, they have no positive copper ions which keep them in a wire. However, this pure negative charge is kept together by the pinch effect i.e. parallel electric currents attract each other and form a minimal (circular) cross section. The round spot on the scree ...
5-th_state_matter - The 5th state of matter
5-th_state_matter - The 5th state of matter

... should electrostatically explode in vacuum, they have no positive copper ions which keep them in a wire. However, this pure negative charge is kept together by the pinch effect i.e. parallel electric currents attract each other and form a minimal (circular) cross section. The round spot on the scree ...
Galaxy Powerpoint Notes
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... Galaxy collisions : Galaxy collisions The Big Band Theory states that the Universe began a long time ago, with galaxies and early stars forming just after. It also states that the Universe is still expanding today, meaning that the galaxies that we see today are travelling at high speeds. Eventuall ...
15-3 Notes: Galaxies
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... Astronomers classify a galaxy as a spiral, elliptical, or irregular galaxy according to its shape. Spiral galaxies, such as the Andromeda galaxy, have a bulge at the center and spiral arms. The spiral arms are made up of gas, dust, and new stars that have formed. The galaxy in which we live is a spi ...
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... 2,000 galaxies. Clusters of galaxies are organized into even larger superclusters—clusters of clusters. Superclusters show organization on the largest scales we can currently observe; they form an intricate web of strings and voids throughout the visible universe. Just think about the quantity of e ...
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... integrated stellar mass in the universe increases gradually throughout this time suggesting that galaxy formation does not happen all at once. 3. Galaxies at high redshifts are peculiar and are likely undergoing mergers. The transition from mergers to normal Hubble types occurs at about z~1.5. Calcu ...
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... The existence of gravitational waves is one of the most intriguing predictions of the General Theory of Relativity proposed by Albert Einstein in 1915. General Relativity { the most accurate theory of gravity available { describes gravity as the curvature of the spacetime, produced by mass-energy co ...
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... a star and it is very similar to billions of other stars in the universe. It has many objects orbiting around it that are held in their orbits by gravity. The solar system is an example of a planetary system. Most of the planets have one or more objects orbiting around them. These are called moons. ...
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... on the grounds that the worst possible idea is to restrict methodologies before you even start your research. and he really attacks the idea that there can be only two roads to truth, or some sort of synthesis of them (as in kant and hegel). ...
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... White dwarfs and neutron stars: physical properties and observational manifestations. Extragalactic radio sources, relativistic jets, and supermassive black holes. Particle acceleration and radiative processes in hot plasmas. Accretion phenomena. X-ray and gamma-ray astrophysics. Requisites: Prerequ ...
Signals from the Beginnings of the World - Max-Planck
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... have put forward at least 150 different theories – most of which have since been dismissed. The issue is further complicated by two sub-classes that were discovered through Compton measurements: gamma-ray bursts with a short duration of less than one to two seconds, and those that typically last bet ...
April 2015 - Southern Astronomical Society
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... been shown to be insubstantial — passing through itself as well as everything else. A study of data returned from NASA’s Hubble Space Telescope and the ESA’s Chandra X-ray Observatory has found dark matter does not slow down when it collides with itself. This is significant as it shows the ghostly s ...
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... flame sweeps through the WD in ~2 s. Most fuel burnt into iron-group elements in these 2 s. ~0.1-0.4 M☼ IME formed in outer less dense regions. Burning and WD hydro expansion rate are about the same. This leads to significant dependence of the 56Ni produced on ignition conditions. Both peak luminosi ...
Chapter 1: Our Place in the Universe
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Astronomy 140 Lecture Notes, Spring 2008 c
Astronomy 140 Lecture Notes, Spring 2008 c

... for Fλ , or in Janskies: 1 Jy = 10−26 W/m2 /Hz = 10−23 erg/cm2 /sec/Hz. To actually determine the 0th magnitude flux F◦ is quite difficult, since it requires the comparison of a star with a laboratory standard light source. Stars are much fainter and hotter than lab standards, and are also much furt ...
Study of the X-ray Source Population and the Dark Matter
Study of the X-ray Source Population and the Dark Matter

... Observations with today's X-ray telescopes have revealed X-ray sources in the fields of the dSphs that are satellites of our Milky Way. The study of X-ray source population in these galaxies and their X-ray luminosity function will help us to trace back the sources that were formed ~1 - 10 Gyrs ago ...
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Physical cosmology



Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate. For most of human history, it was a branch of metaphysics and religion. Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to those on Earth, and Newtonian mechanics, which first allowed us to understand those physical laws.Physical cosmology, as it is now understood, began with the development in 1915 of Albert Einstein's general theory of relativity, followed by major observational discoveries in the 1920s: first, Edwin Hubble discovered that the universe contains a huge number of external galaxies beyond our own Milky Way; then, work by Vesto Slipher and others showed that the universe is expanding. These advances made it possible to speculate about the origin of the universe, and allowed the establishment of the Big Bang Theory, by Georges Lemaitre, as the leading cosmological model. A few researchers still advocate a handful of alternative cosmologies; however, most cosmologists agree that the Big Bang theory explains the observations better.Dramatic advances in observational cosmology since the 1990s, including the cosmic microwave background, distant supernovae and galaxy redshift surveys, have led to the development of a standard model of cosmology. This model requires the universe to contain large amounts of dark matter and dark energy whose nature is currently not well understood, but the model gives detailed predictions that are in excellent agreement with many diverse observations.Cosmology draws heavily on the work of many disparate areas of research in theoretical and applied physics. Areas relevant to cosmology include particle physics experiments and theory, theoretical and observational astrophysics, general relativity, quantum mechanics, and plasma physics.
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