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Estudio de Cúmulos de Galaxias en el Sloan Digital Sky Survey
Estudio de Cúmulos de Galaxias en el Sloan Digital Sky Survey

... – Building Galaxy Merger Trees. ...
Research proposal uploaded for ESO fellowship
Research proposal uploaded for ESO fellowship

Emergency Substitute class orders
Emergency Substitute class orders

Introduction to Galaxies - West Jefferson Local Schools
Introduction to Galaxies - West Jefferson Local Schools

ATA2010
ATA2010

The Fundamental Plane, Stellar Popula6ons
The Fundamental Plane, Stellar Popula6ons

... Some
of
the
(many)
things
we
don’t
know
(at
least
not
well)…
 What
is
the
relaBon
between
stellar
mass
and
dynamical
mass,
 and
how
does
this
vary
with
parent
halo
mass
&
environment?
   How
do
the
observed
trends
in
stellar
populaBons
vary
with
 ...
STEPHAN`S QUINTET
STEPHAN`S QUINTET

The Milky Way Galaxy
The Milky Way Galaxy

... Center of Milky Way Galaxy Apparently, there is an enormous black hole at the center of the galaxy, which is the source of these phenomena An accretion disk surrounding the black hole emits enormous amounts of radiation Observations on three stars that are orbiting the core region at a distance ran ...
Here
Here

... pixels. It is possible to do photometry (the image recorded is then a portion of the sky/star/galaxy) or spectroscopy (the light is dispersed by using a grating into its colors). There are some common problems with CCDs, which need to be taken into account in every observational program: -read-out n ...
The Milky Way Galaxy
The Milky Way Galaxy

Absolute magnitude of type Ia supernovae
Absolute magnitude of type Ia supernovae

26.4 Groups of Stars
26.4 Groups of Stars

... The Milky Way’s flattened disk shape is caused by its rotation. The sun takes about 220 million years to complete one orbit around the galaxy’s center. Recent evidence suggests that there is a massive black hole at our galaxy’s center. Stars are forming in the galaxy's spiral arms. ...
First Light for May, 2001 - South Bay Astronomical Society
First Light for May, 2001 - South Bay Astronomical Society

... The transit method can only find systems that are aligned with our line of sight. The Stellar Wobble Method can find planetary systems that are not fully aligned with our line of sight but still have a component that provides a relative motion towards or away from Earth. Thus, the Wobble method pro ...
슬라이드 1
슬라이드 1

ppt document - FacStaff Home Page for CBU
ppt document - FacStaff Home Page for CBU

Active Galactic Nuclei: are they important?
Active Galactic Nuclei: are they important?

... •Massive central black holes are in all galaxies •In most galaxies the activity is low (e.g. Sgr A* in the Milky Way) but there is no strict border between AGN and non-active galaxies •Thus again BH and galaxies likely evolve ...
telescope as time machine - Galaxy Evolution Explorer
telescope as time machine - Galaxy Evolution Explorer

... gather galactic light that has been journeying toward us for nearly the entire history of the universe. ...
Galaxies - WordPress.com
Galaxies - WordPress.com

PDF format
PDF format

... d)  It depends on the standard candle: if they are Cepheid variables, they will still pulsate at the same rate no matter what distance they are from you. © 2014 Pearson Education, Inc. ...
POISE AND EVOLUTION OF THE GALAXY : STRUCTURE ,
POISE AND EVOLUTION OF THE GALAXY : STRUCTURE ,

An Analysis of Collisional Ring Galaxies
An Analysis of Collisional Ring Galaxies

Document
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... • Interstellar gas clouds emit intense microwaves at specific frequencies. • Doppler shift gives speed • True speed plus proper motion gives distance • Maybe 10s of Mpc but new technique ...
Blowin` in the wind: both `negative` and `positive` feedback in an
Blowin` in the wind: both `negative` and `positive` feedback in an

... We have recently completed two follow-up programs on obscured quasars pre-selected for being in a significant outflowing phase. The first consists in X-Shooter observations of a sample of X-ray selected obscured QSOs at z ∼ 1.5, selected from the XMM-COSMOS survey on the basis of their observed red col ...
First Stars, Quasars and Reionization Observations
First Stars, Quasars and Reionization Observations

... – Pop II: [Fe/H] poor stars, spiral galaxy halos and elliptical galaxies ...
printer-friendly sample test questions
printer-friendly sample test questions

... Interpreting the organization of the above graphic suggests that Aristotle believed each of the following EXCEPT A. all stars are the located the same distance from Earth. B. the Sun is a big star closer to Earth than the other stars. C. stars are found a little beyond the orbit of the last planet. ...
< 1 ... 19 20 21 22 23 24 25 26 27 ... 60 >

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.
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