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Cosmological dynamics with non-minimally coupled scalar field and
Cosmological dynamics with non-minimally coupled scalar field and

CRAZY ILLUSIONS can be created by the power of gravity. Objects
CRAZY ILLUSIONS can be created by the power of gravity. Objects

... a star does the lensing, for example, the images are so close together that even the best telescopes cannot resolve them. This so-called microlensing effect is nonetheless measurable. Because the star is moving, the lens configuration— and therefore the magnification— changes over time. If observers ...
02-02Stars_Part_One
02-02Stars_Part_One

... size, temperature, and distance. -1 is bright, 6 is dim •Absolute magnitude: Apparent magnitude at a distance of 10 parsecs. Factor of only size and temperature ...
Lecture 9a: More on Star formation and evolution 10/22
Lecture 9a: More on Star formation and evolution 10/22

... classes (O B A F G K M)… – Spectral classes are correlated with temperature, that is determined from the peak wavelength of “blackbody” ...
Agreement with Indefinite Pronouns B
Agreement with Indefinite Pronouns B

... The following indefinite pronouns are plural: both, few, many, several. The indefinite pronouns all, any, more, most, none, and some may be either singular or plural, depending on their meaning in a sentence. ...
AP Physics B Waves and Optics Sample MC
AP Physics B Waves and Optics Sample MC

Major constellations
Major constellations

... 11 stars and 5 galaxies. Leo is the Nemean Lion which was killed by Hercules on one of his great quests. Legend says that the lion had a hide that could not punctured by iron, bronze or stone. Since he couldn't reason with the ferocious beast, Hercules strangled it to death and the local people were ...
Stars and gravity - Hyde Park 3rd Grade
Stars and gravity - Hyde Park 3rd Grade

... The Sun is a ball of hot, glowing gases called plasma. It is a star. The Sun looks larger and brighter than stars you see at night because it is a lot closer to Earth. How big is the Sun? Large enough to fit one million Earths inside of it! Wider than the length of 15,000,000 football fields! The te ...
Lecture Nine (Powerpoint format) - Flash
Lecture Nine (Powerpoint format) - Flash

...  Sirius B turns out to be an eclipsing binary, so that its radius can also be determined from the eclipse measurements.  These observations revealed a highly unusual structure -- a mass about that of the sun, and a radius about that of the Earth.  Sirius B became the first-known white dwarf star. ...
Spectra of Underwater Light-Field Fluctuations in the Photic Zone
Spectra of Underwater Light-Field Fluctuations in the Photic Zone

... This is in good agreement with the appearance of the sharp peak occurring in the 4-meter spectrum. There are, of course, other benefits to this kind of analysis of irradiance data which do not contribute to the biological application discussed above, but should be briefly discussed for the sake of c ...
Dark Matter
Dark Matter

10. Molecules and Solids
10. Molecules and Solids

... photons and make transitions to a higher vibrational state when electromagnetic radiation is incident upon a collection of a particular kind of molecule. ...
IV. ASTRONOMY: THE SUN and the MOON
IV. ASTRONOMY: THE SUN and the MOON

... attraction of their constituent particles. 1. There are about 400 billion stars in our Milky Way Galaxy. The Sun is typical in size, but much closer to us than any other star. 2. The very hot, dense, ionized inner parts of a star emit continuous radiation (a “continuum”); many physical processes sme ...
Quantum Physics - StrikerPhysics
Quantum Physics - StrikerPhysics

... phenomena they cannot see or measure directly. ...
grade vii and viii - Sacred Heart CMI Public School
grade vii and viii - Sacred Heart CMI Public School

... Due to their higher boiling points, only metals and silicates could exist in solid form in the warm inner Solar System close to the Sun, and these would eventually form the rocky planets of Mercury, Venus, Earth, and Mars. Because metallic elements only comprised a very small fraction of the solar ...
Numerical Evolu4on of Soliton Stars
Numerical Evolu4on of Soliton Stars

... How
do
we
know
there
is
dark
maPer
 •  Theore.cal:
The
cri.cal
density
is
needed
for
 infla.on
and
its
predic.ons
to
work.
Luminous
 maPer
is
5%
of
this.
There
must
be
non‐ luminous
stuff.
If
70
%
is
dark
energy
then
25%
 must
be
dark
maPer.
 •  
Rota.on
curves
of
stars
shows
the
speeds
do
 not
match ...
Experimental proposal for electromagnetically
Experimental proposal for electromagnetically

... The leftmost one is what we call a single crystal, that is, it is highly perfect which gives rise to its transparency. The center one is composed of numerous and very small interconnected single crystals that the boundaries between these small crystals scatter a portion of the light reflected from t ...
Galaxies and Active Galaxies
Galaxies and Active Galaxies

... – Works only for the nearby galaxies. ...
Presentazione di PowerPoint
Presentazione di PowerPoint

... After the starting guesses of the centroids (FIND) and brightness (PHOTOMETRY) are measured, and the PSF model determined (PSF), the PSF is first shifted and scaled to the position and brightness of each star, and each profile is subtracted, out to the profile radius, from the original image. This ...
Extended Infrared Emission from LIRGs
Extended Infrared Emission from LIRGs

... (GOALS; Armus et al. 2009) of 202 systems (181 of which are LIRGs) All systems are observed with all four Spitzer/IRS modules (5-37μm) Apply an upper limit on distance (<85 Mpc) in order for the IRS slit size to correspond to a projected distance < 1.5kpc (best case is 0.26kpc) A total of 93 galaxie ...
Lecture 22 - Seattle Central
Lecture 22 - Seattle Central

... The iron core gets crushed so that it’s no longer iron, the electrons and protons combine into neutrons, the volume of the core reduces by a factor of 1018 Outer core falls in at about 25% of the speed of light, the core ...
Modern physics
Modern physics

... • Bohr used deBroglie’s matter waves, quantized angular momentum, for better H atom model. En = E/n2 • Bohr model explained observed H spectra, derived phenomenological Rydberg constant • Quantum numbers n, l, ml (Zeeman effect) • Solution to Schrodinger equation showed that En = E/l(l+1) • Pauli p ...
Slide 1
Slide 1

... • Limited by the energy of the SN and the surrounding gas density and temperature • Identified as HII (ionized hydrogen) regions- ionized shockfronts. ...
How much Sugar in Gum
How much Sugar in Gum

... Background and Misconceptions: Since the distances are vast in the solar system and between stars, astronomers have created various units to represent these large distances. They use them only because they are easier to use and they are agreed upon quantities. The common units are: ...
Hour of the Stars
Hour of the Stars

... Christian Berg gives sound to the landform. Yet silence reigns. Light direction makes visible the bodies rolling silently over the wooden bridge. Elusive, then clearer, closer, more corporeal, as they come towards us; the reverse as they move away from us. Always, they remain in the bosom of the nig ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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