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The Flow of Energy Out of the Sun
The Flow of Energy Out of the Sun

... A sub-microscopic simulation, called Interaction, allows you to study how an individual line or continuum photon interacts with atoms. The Line Formation simulation demonstrates how photons that have just the right amount of energy to kick an electron of a gas atom to a higher energy state are absor ...
Rosolowsky
Rosolowsky

exploring fundamental physics with neutron stars
exploring fundamental physics with neutron stars

... gravity into a spherical volume 20-30 km in diameter, spinning around their axis up to a thousand times per second, shining in the soft X-ray, with a powerful magnetosphere generated by magnetic fields more than a billion times stronger than those in the Sun. This magnetosphere, which is like an ext ...
Farthest Neighbor: The Distant Milky Way Satellite Eridanus II
Farthest Neighbor: The Distant Milky Way Satellite Eridanus II

EXPLORING FUNDAMENTAL PHYSICS WITH NEUTRON STARS
EXPLORING FUNDAMENTAL PHYSICS WITH NEUTRON STARS

... gravity into a spherical volume 20-30 km in diameter, spinning around their axis up to a thousand times per second, shining in the soft X-ray, with a powerful magnetosphere generated by magnetic fields more than a billion times stronger than those in the Sun. This magnetosphere, which is like an ext ...
Andromeda *ruler of men*
Andromeda *ruler of men*

The Main Sequence - University of Arizona
The Main Sequence - University of Arizona

... 17O(p,)18F 18F(-,)18O 18O(p,)19F 19F(p,)16O ...
a spectral performance model for the
a spectral performance model for the

... layers. This design method and use of materials provides an equivalent index that can approximate to the original substrate refractive index at its outer surface, matching well to the CdTe and providing a good index match for the application for a broadband antireflection coating. The ultra-wide bro ...
Cosmo-PST
Cosmo-PST

... by mutual gravitational attraction of the galaxies. • Fate of the universe depends on the matter density in the universe. • Define “critical density”, rc, which is just enough to slow the cosmic expansion to a halt at infinity. ...
Celestron Manual
Celestron Manual

... Take time to read through this manual before embarking on your journey through the Universe. It may take a few observing sessions to become familiar with your telescope, so you should keep this manual handy until you have fully mastered your telescope’s operation. The manual gives detailed informati ...
Phase Transitions of the First Kind as Radiation
Phase Transitions of the First Kind as Radiation

theoretical and experimental study of spectroscopic characteristics
theoretical and experimental study of spectroscopic characteristics

Computation of diffraction patterns Part 1
Computation of diffraction patterns Part 1

... II. The other big structural change can be seen in the first and last lines. The script has been turned into a MATLAB function. When you want to do the calculations it contains you call it like this. Caution: the global variables must still be set. >> [yd Itot] = Huygens; and MATLAB will generate t ...
The Sun`s journey through the local interstellar medium: the
The Sun`s journey through the local interstellar medium: the

PDF Link
PDF Link

... many situations when this condition is not met in practice. For example, interference between multiple waves may generate power spectra that exhibit multiple maxima and minimums and are, thus, noninjective. A laser resonator is a common example whereby the spatial power spectrum is not injective and ...
Novel sol-gel material for fabrication of a long period waveguide
Novel sol-gel material for fabrication of a long period waveguide

... replica-molding lithography and shortened as soft-lithography, appeared [10]. In the soft-lithography technique, a mechanically flexible and elastomeric Poly (di-methylsiloxane) (PDMS) mold stamp was used to transfer the desired pattern because its relatively low surface energy results in weak adhes ...
Gravitational waves - LIGO
Gravitational waves - LIGO

WASP-86b and WASP-102b: super-dense versus bloated planets
WASP-86b and WASP-102b: super-dense versus bloated planets

... WASP-102b shows a larger than model-predicted radius, indicating that the planet is receiving a strong incident flux which contributes to the inflation of its radius. On the other hand, with a density of ρpl = 3.24± 0.3 ρJ , WASP-86b is the densest gas giant planet among planets with masses in the r ...
Silicon-on-Insulator Grating Duplexer for Fiber-to-the
Silicon-on-Insulator Grating Duplexer for Fiber-to-the

... duplexing operation and fiber-to-chip interfacing is presented in figure 1. It consists of a one-dimensional grating structure defined on an SOI waveguide platform. The single mode optical fiber is tilted by an angle θ with respect to the vertical axis. While in standard fiber-to-waveguide grating c ...
The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument
The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument

... IRIS has three distinct optical units that occur sequentially after the adaptive optics focal plane. At the top of the instrument are the on-instrument wavefront sensors (OIWFS) which monitor up to three stars across a 2 arcmin region of the AO corrected field. Their primary purposes are to remove i ...
The Demonstration
The Demonstration

... (floating on the water). If the refractive indices of the water and the oil are made to be the same there is no 2nd refraction since there is no discontinuity in the refractive property. When we don’t have this second reflection we don’t see the colors. The existence of this coloring effect depends ...
analysis of eclipsing binary data - Astrophysics
analysis of eclipsing binary data - Astrophysics

Spectra of Cosmic Ray Protons and Helium Produced in Supernova
Spectra of Cosmic Ray Protons and Helium Produced in Supernova

... cosmic ray halo boundaries into intergalactic space, where cosmic ray density is negligible. We employ the plain diffusion model with a flat cosmic ray halo (Ginzburg & Ptuskin 1976; Strong et al. 2007) for calculations of cosmic ray propagation in the Galaxy. The leaky-box approximation to the diff ...
A model of low-mass neutron stars with a quark core
A model of low-mass neutron stars with a quark core

UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to
UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to

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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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