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Galaxies – Island universes
Galaxies – Island universes

... • If a small galaxy has a central collision with a larger spiral galaxy, the gravitational pulse can compress gas/dust and make a star formation burst in a ring. • Collision energy added to the central bulge can stretch it out into a very non-spherica ...
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... in nebulae (the plural of nebula) is mostly hydrogen gas (H2). ...
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PPT - ICRA
PPT - ICRA

... 2) ``Melting’’ phase transition: the nucleon matter core, nuclei matter surroundings. 3) Super-critical electric field on the surface of collapsing core. 4) Electron-positron-photon plasma (dyadosphere) formed in gravitational collapses. 5) Hydrodynamic expansion of Electron-positron-photon plasma. ...
stars & galaxies
stars & galaxies

... The milKy Way… our home iN The sTars… • The Milky Way has a diameter of about 100,000 light years. • The nucleus is 2000 light years thick. • Our sun is located 30,000 light years from the nucleus. • It takes the sun 200 million years to ...
Our Galaxy -- The Milky Way PowerPoint
Our Galaxy -- The Milky Way PowerPoint

... – Gravitational bending of light has been observed • Tentatively, MACHOs account for < 40% of dark matter ...
Cosmology - RHIG - Wayne State University
Cosmology - RHIG - Wayne State University

... • Connected with the quark masses • When confined quarks have a large dynamical mass constituent mass • In the small coupling limit (some) quarks have small mass current mass ...
The Main Features of the X
The Main Features of the X

... Thermal bremsstrahlung or free-free emission occurs when an e- is accelerated due to the strong electrical attraction of a positive ion in a plasma. Temperatures above 105 K are ...
Research proposal uploaded for ESO fellowship
Research proposal uploaded for ESO fellowship

... global star formation rate decline of the universe? Supernova feedback represents a long standing problem in galaxy formation model. Currently, toy models are used to treat supernova feedback, which are parametrized to reproduce the faint-end of the luminosity function (Cole et al. 2000; Guo et al. ...
What Do We Really Know About the Universe?
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Spiral Galaxies - Astronomy Centre
Spiral Galaxies - Astronomy Centre

... Nature of the Nebulae • We now know that Kant was correct • Our Milky Way Galaxy is just one of Kant’s island universes, which are now referred to as galaxies • The word Universe now refers to the full expanse of space and its contents • While most diffuse nebulae are nearby clouds of gas and dust ...
How Big is the Universe
How Big is the Universe

... Andromeda. One particular type of star allowed him to calculate its distance. He showed that the Andromeda Nebula was far outside our Milky Way Galaxy. Hubble realized that many of the objects that astronomers called nebulae were not actually clouds of gas. They were what we now call galaxies – a co ...
Galaxies Powerpoint
Galaxies Powerpoint

... gas, and dust in space that are held together by gravity. • The largest galaxies contain more than a trillion stars. Smaller galaxies may have only a few million. • Scientists estimate the number of stars from the size and brightness of the galaxy. ...
Main Types of Galaxies
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... gas, and dust in space that are held together by gravity. • The largest galaxies contain more than a trillion stars. Smaller galaxies may have only a few million. • Scientists estimate the number of stars from the size and brightness of the galaxy. ...
Assignment 10
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Pistol Star - University of Dayton
Pistol Star - University of Dayton

... Earth is only one planet orbiting one star among roughly a hundred billion stars in our Milky Way Galaxy. The Milky Way is only one galaxy of billions in the universe. Looking beyond the solar system into galactic and intergalactic space, we must stretch our minds to nearly unimaginable distances t ...
relativistic time correction on movement of distant galaxies
relativistic time correction on movement of distant galaxies

... stars. Suppose there is a Sun like star of about 5 billion years old, then that star was formed at about 13.4+5=18.4 billion years ago. (In fact, present age of this star is to be multiplied by 1+z =1.98. So it is 5x1.98= 9.9 billion light years. But we have just received light from that galaxy and ...
Galaxies and the Universe
Galaxies and the Universe

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Answers for the HST Scavenger Hunt
Answers for the HST Scavenger Hunt

... The spherical outer boundary of a black hole. Once matter crosses this threshold, the speed required for it to escape the black hole’s gravitational grip is greater than the speed of light. When scientists used the HST to study Cygnus X-1, they were able to observe two of these events, which defines ...
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Universe 8e Lecture Chapter 24 Galaxies

... Hot intergalactic gases in rich clusters account for a small part of the unobserved mass. These gases are detected by their X-ray emission. The remaining unobserved mass is probably in the form of dark-matter halos that surround the galaxies in these clusters. Gravitational lensing of remote galaxie ...
Chapter14- Our Galaxy - SFA Physics and Astronomy
Chapter14- Our Galaxy - SFA Physics and Astronomy

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The Bible and big bang cosmology
The Bible and big bang cosmology

... “The stars of our own galaxy, the Milky Way, rotate about the galactic center with different speeds, the inner ones rotating faster than the outer ones. The observed rotation speeds are so fast that if our galaxy were more than a few hundred million years old, it would be a featureless disc of stars ...
Stellar Pops 2
Stellar Pops 2

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(Mike Riddle CTI)-84_eng_cr_v4.0
(Mike Riddle CTI)-84_eng_cr_v4.0

... “The stars of our own galaxy, the Milky Way, rotate about the galactic center with different speeds, the inner ones rotating faster than the outer ones. The observed rotation speeds are so fast that if our galaxy were more than a few hundred million years old, it would be a featureless disc of stars ...
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Structure formation

In physical cosmology, structure formation refers to the formation of galaxies, galaxy clusters and larger structures from small early density fluctuations. The Universe, as is now known from observations of the cosmic microwave background radiation, began in a hot, dense, nearly uniform state approximately 13.8 billion years ago. However, looking in the sky today, we see structures on all scales, from stars and planets to galaxies and, on still larger scales still, galaxy clusters and sheet-like structures of galaxies separated by enormous voids containing few galaxies. Structure formation attempts to model how these structures formed by gravitational instability of small early density ripples.The modern Lambda-CDM model is successful at predicting the observed large-scale distribution of galaxies, clusters and voids; but on the scale of individual galaxies there are many complications due to highly nonlinear processes involving baryonic physics, gas heating and cooling, star formation and feedback. Understanding the processes of galaxy formation is a major topic of modern cosmology research, both via observations such as the Hubble Ultra-Deep Field and via large computer simulations.
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