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Interactive 4 - Hertzsprung-Russell Diagram Explorer
Interactive 4 - Hertzsprung-Russell Diagram Explorer

... @citcvc [email protected] Yr 11 Cosmic Engine with Answers ...
Starburst Galaxies Under the Microscope: High
Starburst Galaxies Under the Microscope: High

... imaging in a number of narrow-band filters in the N-band, and long-slit spectroscopy with a 0.75 slit, covering the two most prominent clusters. Some key results are shown in Figures 1 and 2 (Snijders et al. 2006), which show a number of surprising results. In the first place, the Eastern cluster i ...
ppt document - FacStaff Home Page for CBU
ppt document - FacStaff Home Page for CBU

... By using the doppler effect on spectra, we can determine the motion of light emitting objects towards (blue shift) or away (red shift) from us. It is only possible to determine the sideways motion of objects if they are close enough and move fast enough to make a measurable angular change in their l ...
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PDF - Interactive Stars

A Detailed Derivation of the Radial Velocity Equation
A Detailed Derivation of the Radial Velocity Equation

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Your Astrology Defense Kit
Your Astrology Defense Kit

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Planetary rulers are not simple affinities
Planetary rulers are not simple affinities

The Circumstellar Medium of Massive Stars in Motion
The Circumstellar Medium of Massive Stars in Motion

... stellar space velocities, produces a huge diversity of circumstellar structures. Many of the closest such structures, such as the CSM of Betelgeuse and ζ Oph, have been observed in great detail with modern observatories, and yet we still do not have a definitive understanding of these objects. The u ...
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The motions of the Earth

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Here`s - Abrams Planetarium

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Earth-Sky Relationships and the Celestial Sphere

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Astronomy Astrophysics First detection of the field star overdensity in the Perseus... &

... the two sets of physical parameters. This cleanest sample contains 8328 stars and is named CS-MB or CS-EC depending on whether their physical parameters were computed using the MB or EC method (see Fig. 1). This sample contains stars with more accurate SPP data, but has fewer statistics owing to the ...
PDF - Interactive Stars
PDF - Interactive Stars

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ISS Sighting Opportunities

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Test 3 Review Clicker Questions

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Sample pages 1 PDF

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Scientific Evidence for A
Scientific Evidence for A

... was so. And God made the beasts of the earth after their kind, and the cattle after their kind, and everything that creeps on the ground after its kind; and God saw that it was good. Then God said, “Let Us make man in Our image, according to Our likeness; and let them rule over the fish of the sea a ...
Nulling Interferometer
Nulling Interferometer

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Black Holes in Binary Systems and Galaxy Nuclei
Black Holes in Binary Systems and Galaxy Nuclei

... A big progress in observations of stellar mass BHs and supermassive BHs has been achieved during last 40 years. Hundreds of reliable BH candidates have been discovered up to now. All observational appearances of BH candidates are in excellent agreement with Einstein General Relativity. Taking into a ...
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The old globular cluster system of the dIrr galaxy NGC 1427A in the

... that all three dwarf galaxy types host a population of old GCs with very similar (V − I) colors. The mean color of this population is almost identical to the (V − I) colors of the blue GC population in massive early-type galaxies. One way to address the evolutionary connection between dE, dSph, dIrr ...
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Catching Planets in Formation with GMT

... Size: ~7 X 7 Deg (cloud core plus extended region)  GMACS FOV: 8 x 18’  NIRMOS FOV:5.5 x 5.5’ IMACS limiting magnitude I~21.5, S/N=30, in 4 hr @ R~2000 10-4 Lsun or 3- 5MJ 15% too faint (>21.5) for IMACS ...
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Dynamical Mass Measurements of Pre-Main

... There are now 23 dynamical mass measurements for pre-main-sequence (PMS) stars of less than 2 M , with most of the measured stars having masses greater than 0.5 M . The masses of two PMS brown dwarfs have also been precisely measured. The most important application of these dynamical mass measuremen ...
PDF Full-text
PDF Full-text

... spectrum of the M star seen by an exoplanet in the habitable zone is more than three orders of magnitude fainter than the solar radiation received at Earth. On the other hand, the FUV emission of both stars formed in their chromospheres are comparable in flux. Thus while M stars are faint in the NUV ...
Brightness and Flux Density
Brightness and Flux Density

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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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