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Structure and optical properties of reconstructed Si and Ge surfaces
Structure and optical properties of reconstructed Si and Ge surfaces

... as the forces on the bulk atoms are not similar to those on surface atoms. This is called surface reconstruction. When these systems are energetically relaxed, sometimes they form special ordered structures such as one dimensional atomic chains or rows of dimers etc. due to surface reconstruction. S ...
The Dark Matter Problem
The Dark Matter Problem

... ”’You do not know the Power of the Dark Side. Join me, and together we can use dark matter to make galaxy rotation curves flat.’ I often hear this sort of paternalistic line from well intentioned senior astronomers. My response is the same as Luke's, with analogous consequences for my career.” ...
the discovery of a massive cluster of red supergiants with glimpse
the discovery of a massive cluster of red supergiants with glimpse

... and energetic photons from young massive stars. Infrared dark clouds (IRDCs) and dark filaments appear superimposed on the bright diffuse background at many locations across this field, indicating the presence of opaque, cold clouds in the foreground. A handful of very red and bright sources, often ...
Model SEDs of Massive YSOs
Model SEDs of Massive YSOs

... Accretion Disk Stage -- Class II ...
A laser motor directly transforms light energy into mechanical
A laser motor directly transforms light energy into mechanical

... technique can only apply forces in the pN range. It is estimated that only about 10−10 % of the light energy is used for driving the object.3 Hence, if the efficiency of converting light into mechanical energy could be improved, a new range of applications could emerge. The light energy is actually ...
Chapter 14
Chapter 14

... Eventually, the star gets so hot that its radiation ionizes the surround gases and vaporizes the dust. When this happens, surrounding material becomes transparent. The protostar then begins to shine much brighter than before. However it does so erratically, since clouds of gas and dust are still mov ...
Spiral Galaxies: Density Waves
Spiral Galaxies: Density Waves

galaxy solar system supernova
galaxy solar system supernova

... 1. An astronomer is a scientist who studies planets, stars, galaxies, and other objects in space. 2. You would expect an astronomer to use a telescope. 3. She wants to be an astronomer someday, so she is taking many science classes in college. ...
Fluorescence: Fluorescence studies prone to self
Fluorescence: Fluorescence studies prone to self

ppt - Institute for Astronomy
ppt - Institute for Astronomy

... The separations of the above FUor pairs are so large that it would take several thousand years from a periastron passage to reach their present locations. FUor eruptions probably do not last that ...
Resolution-and throughput-enhanced spectroscopy using high
Resolution-and throughput-enhanced spectroscopy using high

... used to solve Eq. 1, and is performed until convergence. For this study, a computational slit function S corresponding to a 5µm slit was used. By utilizing a computational slit with a width narrower than the physical entrance aperture, the idea is that the spectral resolution of the resulting spectr ...
Circumstellar
Circumstellar

... VY CMa -- the extreme red supergiant, powerful OH/IR source mass loss rate 4 x 10-4 Famous asymmetric red nebula, > 10” across, visible in small ground based telescopes. HST/WFPC2 images revealed complex environment – numerous knots, filamentary arcs, prominent nebulous arc Due to multiple, asymmet ...
Photoelectric Effect Lab
Photoelectric Effect Lab

Supernovae and supernova remnants
Supernovae and supernova remnants

... supernova, the entire star is detonated while in others a compact object – a black hole or a neutron star – is left behind. The metal abundance in the universe is referred to as the ‘cosmic abundance’, which is essentially the same as the abundances of the elements within our solar system. These abu ...
Astronomy Astrophysics
Astronomy Astrophysics

Today in Astronomy 102: electron degeneracy pressure and white
Today in Astronomy 102: electron degeneracy pressure and white

refraction ppt_2010
refraction ppt_2010

... Note the reflection of the man facing her. He must be you! Because reflection shows that he is directly in front of the woman, and thus he must be the viewer of the painter. You are looking into Manet’s work and seeing your reflection well off to your right. The effect is errie because it is not wha ...
Dust in Space - Max-Planck
Dust in Space - Max-Planck

... The further away a galaxy is, however, the more difficult verification becomes. It was thus hailed as a great breakthrough when, a few years ago, scientists succeeded in measuring the thermal emission of dust in the most distant known quasars. The latter are the ultrabright central regions of galaxi ...
Chapter 33. Electromagnetic Waves
Chapter 33. Electromagnetic Waves

... • Wavelength λ is the horizontal distance between any two successive equivalent points on the wave. • Amplitude A is the highest point on the wave pattern. • Period T is the time required for the wave to travel a distance of one wavelength. Unit is second. • Frequency f : f=1/T. The frequency is mea ...
Stellar Evolution
Stellar Evolution

Structure of the hot object in the symbiotic prototype Z And during its
Structure of the hot object in the symbiotic prototype Z And during its

... 3.0.7, 3.0.8 and 2.4.1. We used the calibrated time-tag observations (TTAG photon collecting mode) taken through the large aperture (LWRS). Before adding the flux from all exposures we applied an appropriate wavelength shift relative to one to obtain the best overlap of the absorption features. Then ...
To understand the deaths of stars and how it depends on
To understand the deaths of stars and how it depends on

Reverse Iontophoresis - Faculty Server Contact
Reverse Iontophoresis - Faculty Server Contact

... will cause variations in its index of refraction  The refractive index can be measured by interferometry ...
Document
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... Cut along solid black line to make a strip. Fold on dashed. ...
Accretion Processes of Binaries of White Dwarfs
Accretion Processes of Binaries of White Dwarfs

... 2. SPH simulations show that steady accretion disk can be formed via gravitational capture of slow stellar wind ...
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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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