Galaxy clusters - University of Iowa Astrophysics
... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
Galaxy clusters - University of Iowa Astrophysics
... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
... • From this, the amount of X-ray emitting gas can be calculated to be 2×1014 M • The mass of X-ray emitting gas is greater than the mass in all the stars in all the galaxies in the cluster and about 10% of the total mass. ...
Astron 104 Laboratory #11 The Scale of the Milky Way
... galaxies. From question 9, we saw that the Andromeda Galaxy was about 2,500,000 ltyr from us. On the picture, this spot would be 250 cm (about two and a half meter sticks) away from the dot representing the Sun. The nearest group of galaxies to us (not counting our own Local Group) is the Virgo Clus ...
... galaxies. From question 9, we saw that the Andromeda Galaxy was about 2,500,000 ltyr from us. On the picture, this spot would be 250 cm (about two and a half meter sticks) away from the dot representing the Sun. The nearest group of galaxies to us (not counting our own Local Group) is the Virgo Clus ...
Type Ia Supernovae in the SDSS Strip 82
... Properties of Host galaxy -(u-r) & (g-r) color -Luminosity -Local density -Distance to r1 ...
... Properties of Host galaxy -(u-r) & (g-r) color -Luminosity -Local density -Distance to r1 ...
The Universe and Galaxies - West Jefferson Local Schools
... - universe - sum of all _________ and energy that ever has, does, and ever will exist everything physical that exists in _________ and _________ - _________ – the study of how the universe began, what it is made of and how it continues to evolve and change - Of what is the universe made / composed ...
... - universe - sum of all _________ and energy that ever has, does, and ever will exist everything physical that exists in _________ and _________ - _________ – the study of how the universe began, what it is made of and how it continues to evolve and change - Of what is the universe made / composed ...
2. Universe and galaxies
... • II. Most common type • III. Contains only old stars and very little dust and gas. ...
... • II. Most common type • III. Contains only old stars and very little dust and gas. ...
Lecture 17: General Relativity and Black Holes
... (a) Stars near the center of the galaxy have very small orbits and very high orbital speeds (b) X-ray flares detected from Sag A* have very short variation timescales. (c) Infrared observations indicate there is a bar at the galactic center. (d) is a very strong source of X-ray and synchrotron emiss ...
... (a) Stars near the center of the galaxy have very small orbits and very high orbital speeds (b) X-ray flares detected from Sag A* have very short variation timescales. (c) Infrared observations indicate there is a bar at the galactic center. (d) is a very strong source of X-ray and synchrotron emiss ...
combined astro show 2013
... The temperature of the gas, generally the spectral lines of various elements become more prominent at certain temperatures ...
... The temperature of the gas, generally the spectral lines of various elements become more prominent at certain temperatures ...
galaxy.
... • The zone of avoidance must be an artifact of something in our galaxyperhaps dust extinction- blocking our view of galaxies in the Milky Way. • S Andromeda was not a normal nova. It was something else, something much brighter. • Slipher’s observations of several spiral nebulae showed that they had ...
... • The zone of avoidance must be an artifact of something in our galaxyperhaps dust extinction- blocking our view of galaxies in the Milky Way. • S Andromeda was not a normal nova. It was something else, something much brighter. • Slipher’s observations of several spiral nebulae showed that they had ...
Messier 87
Messier 87 (also known as Virgo A or NGC 4486, and generally abbreviated to M87) is a supergiant elliptical galaxy in the constellation Virgo. One of the most massive galaxies in the local universe, it is notable for its large population of globular clusters—M87 contains about 12,000 compared to the 150-200 orbiting the Milky Way—and its jet of energetic plasma that originates at the core and extends outward at least 1,500 parsecs (4,900 light-years), travelling at relativistic speed. It is one of the brightest radio sources in the sky, and is a popular target for both amateur astronomy observations and professional astronomy study.French astronomer Charles Messier discovered M87 in 1781, cataloguing it as a nebulous feature while searching for objects that would confuse comet hunters. The second brightest galaxy within the northern Virgo Cluster, M87 is located about 16.4 million parsecs (53.5 million light-years) from Earth. Unlike a disk-shaped spiral galaxy, M87 has no distinctive dust lanes. Instead, it has an almost featureless, ellipsoidal shape typical of most giant elliptical galaxies, diminishing in luminosity with distance from the centre. Forming around one sixth of M87's mass, the stars in this galaxy have a nearly spherically symmetric distribution, their density decreasing with increasing distance from the core. At the core is a supermassive black hole, which forms the primary component of an active galactic nucleus. This object is a strong source of multiwavelength radiation, particularly radio waves. M87's galactic envelope extends out to a radius of about 150 kiloparsecs (490,000 light-years), where it has been truncated—possibly by an encounter with another galaxy. Between the stars is a diffuse interstellar medium of gas that has been chemically enriched by elements emitted from evolved stars.