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The Interior of the Sun
The Interior of the Sun

... The Sun is a ball of hot gas so its interior transmits sound waves very well which can be seen by the doppler shifting of light emitted at the Sun's surface. Helioseismology uses these sound waves to probe the interior of the Sun. It is the same like geologists use seismic waves from earthquakes to ...
White dwarfs from GAIA: The 7th dimension
White dwarfs from GAIA: The 7th dimension

The Sun is our local star.
The Sun is our local star.

... Sunspot activity follows a pattern that lasts about 11 years. At the peak of the cycle, dozens of sunspots may appear. During periods of low activity, there may not be any sunspots. Sunspots move across the Sun’s surface as it rotates. Astronomers first realized that the Sun rotates when they notice ...
ana-phy-ret2016
ana-phy-ret2016

... Some important facts 1. 150 million receptors & 1 million optic nerveconvergence and mixing of visual signals 2. The horizontal action of the horizontal and amacrine cells can allow one area of the retina to control another (e.g., one stimulus inhibiting another). 3. The response of cones to variou ...
How to predict the meridian passage time of a star. This is not an
How to predict the meridian passage time of a star. This is not an

Mar 2016 - Bays Mountain Park
Mar 2016 - Bays Mountain Park

... used. Early scientific instruments were fancy sticks, such as the astrolabe and armillary. The Best Man: America’s Pioneering Astrophysicist, J.E. Keeler Tom English, professor of astronomy at Guilford Technical Community College, gave an in-depth biography of American astrophysicist James Edward Ke ...
Structural Characterization of Photoluminescent Porous Silicon with
Structural Characterization of Photoluminescent Porous Silicon with

Terrestrial aurora - Annales Geophysicae
Terrestrial aurora - Annales Geophysicae

... waves and particles. Particular observations include the fast (Temerin and Roth, 1992; Roth and Temerin, 1997). Both temporal electron and wave oscillations, as shown on Fig. 1, environments have very low β (thermal to magnetic pressure at a frequency of 120 Hz, below the hydrogen H+ gyrofreratio) p ...
Searching for the Secrets of Massive Star Birth
Searching for the Secrets of Massive Star Birth

... active star formation from beyond a few kpc in our own Galaxy to deep into the early universe. The birth of massive stars remains one of the fundamental unsolved topics in astronomy (Zinnecker &Yorke 2007; McKee & Ostriker 2007). Young massive stars are associated with dense gas found predominately ...
Astronomy Astrophysics A VLT/FLAMES survey for massive binaries in Westerlund 1 &
Astronomy Astrophysics A VLT/FLAMES survey for massive binaries in Westerlund 1 &

... driven asymmetries – rather than binary reflex motion – is in any event phased on their known orbital periods (Stevens & Howarth 1999). We are thus confident that the 5.05 day period identified in the RV curve of W239 reflects an underlying binary orbital period of the system. Motivated by this find ...
Slide 1 - Documents
Slide 1 - Documents

... 35 AU, which is related to the KB and SD, in agreement with observations, Fig.b. ...
PDF file - Research in Astronomy and Astrophysics
PDF file - Research in Astronomy and Astrophysics

... HH objects, they originate from optically visible young low mass stars, which apparently suffer very low extinction and are not embedded in opaque molecular cloud cores; (b) probably due to impacts from the strong radiation field encountered, the jets are predominantly one-sided or highly asymmetric ...
Physics 228 Today: Polarization, Scattering
Physics 228 Today: Polarization, Scattering

... light is < 1 μm, we can linearly polarize it using arrays of molecules, as in a polaroid filter. We can think of this similarly to microwaves and the metal plate: if the electric field orientation can accelerate electrons in the material - E is parallel to the long molecules - the electrons will acc ...
The Visual System Ophthalmic Lenses Basic Optical Formulas
The Visual System Ophthalmic Lenses Basic Optical Formulas

... all three primary points in the spectrum must be absorbed to the same degree. When creating a filter by absorbing dye into resin, this process is further complicated by the inconsistent nature of the chemicals involved. ...
Free Electron Lasers
Free Electron Lasers

Hunting for Orphaned Central Compact Objects among Radio Pulsars
Hunting for Orphaned Central Compact Objects among Radio Pulsars

... that there should be over 106 older ones in the Galaxy (Kaspi 2010). This is in contrast to the small number of known radio pulsars with low B ∼ 1010 G as shown in the P -Ṗ diagram in Figure 1, given that there is no observational bias against these pulsars in radio surveys (see Kramer et al. 2003; ...
discovery of four new massive and dense cold cores
discovery of four new massive and dense cold cores

... form of molecular gas, as suggested by the similar values of the mass derived from the dust continuum emission (gas mass) and the virial mass (total mass) determined from the molecular line observations, indicating that the gas dominates the gravitational potential. Although we cannot conclude that ...
News from high-mass twin stars
News from high-mass twin stars

Lecture 21 Wave Optics
Lecture 21 Wave Optics

... a>min=1.22/D, namely the angle of the first dark fringe of the diffraction pattern • Objects not resolvable if a<min • Objects marginally resolvable if amin ...
Name Period Test on Size and Scale from the Electron to the
Name Period Test on Size and Scale from the Electron to the

... The deepest hole in the earth is 7.5 miles dug in Russia. The deepest natural point on earth is in the oceans 6.8 miles . Where is that place and what is the geological form? The highest point on Earth is 29,500 feet(5.5 miles) Where is that and what is the land form. ...
Modeling non-thermal emission from stellar bow shocks
Modeling non-thermal emission from stellar bow shocks

... Assuming the velocity of this star is 67 km s−1 (Kobulnicky et al. 2010), the mass-loss rate 10−5 M⊙ yr−1 (Markova et al. 2004; Repolust et al. 2004), the stellar wind velocity 2300 km s−1 (Howarth et al. 1997), and that the standoff radius is R0 = 1.5 pc (Peri et al. 2012), from Eq. 1 we derive a m ...
chapter5 - Homework Market
chapter5 - Homework Market

... heats it to high temperature—and it glows. • You can also recognize the light emitted by a toaster coil as blackbody radiation. • Many objects in the sky—including the sun—primarily emit blackbody radiation because they are mostly opaque. ...
PDF format
PDF format

... •  An interstellar cloud of gas and/or dust ...
Introduction - Cambridge University Press
Introduction - Cambridge University Press

... type is very closely related to temperature and colour. Temperatures cannot be measured directly for many stars, but colours can be, so the observational H–R diagram is often a plot of MV against colour index (such as B − V ). The theoretical H–R diagram uses quantities more closely related to compu ...
A Treatise on Electricity and Magnetism
A Treatise on Electricity and Magnetism

... body   to   another   by   means   of   a   medium   occupying   the   space   between   them.   The   undulatory2  theory  of  light  also  assumes  the  existence  of  a  medium.  We  have  now  to   show  that  the  properties  of ...
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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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