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Lecture 11 - University of Washington
Lecture 11 - University of Washington

Ground-based variability surveys towards Centaurus A: worthwhile
Ground-based variability surveys towards Centaurus A: worthwhile

... Furthermore, elliptical galaxies tend to live in more dense environments, where galactic encounters are more common and old stellar populations would have been pushed out to larger radii into the halo. Microlensing surveys in elliptical galaxies would also enable the study of these stellar halos, th ...
Document
Document

... to the mass of each object, and inversely proportional to the square of the distance between the two objects. •G is the Universal gravitational constant G, which was measured by Cavendish after more than 100 years ...
WORD - UWL faculty websites
WORD - UWL faculty websites

... Split light up according to wavelength (energy)  see a spectrum of various colors  A continuous spectrum is one where all colors are visible. Hot dense objects (like a bulb filament, or the center of a star) emit this kind of spectrum, producing thermal (blackbody) emission: o Hotter objects produ ...
The Very Small Array (VSA) - Department of Physics
The Very Small Array (VSA) - Department of Physics

REINFORCEMENT Grade 3 EVS FOR SA2
REINFORCEMENT Grade 3 EVS FOR SA2

TP954 - DPTI
TP954 - DPTI

... The acquired spectrum is then compared with the CIE standard illuminant A spectrum (on file) and a correction file generated at 5 nm intervals in the range 380-760nm. ...
The Distance Ladder I - Sierra College Astronomy Home Page
The Distance Ladder I - Sierra College Astronomy Home Page

Letter to the Editor ASTRONOMY ASTROPHYSICS
Letter to the Editor ASTRONOMY ASTROPHYSICS

Stars and Star Patterns
Stars and Star Patterns

... A star is a huge ball of very hot gases like hydrogen and helium. ...
Stellar Mass Assembly History
Stellar Mass Assembly History

... galaxies with significant SF activity progressively decreases. Active star formation in low mass galaxies seems to be (on average) more protracted than in massive galaxies. ...
Stars, Galaxies, and the Universe
Stars, Galaxies, and the Universe

... Chemical elements in a star’s atmosphere absorb light from the star. Each element absorbs light at different wavelengths. Thus by comparing them to other known spectrums of different elements astronomers can infer which elements are found in a star. ...
Broadneck Physics 2010
Broadneck Physics 2010

... useful. In 1303, French physician Bernard of Gordon wrote of the use of lenses to correct eyesight. Around 1610, Galileo used two lenses to make a telescope, with which he discovered the moons of Jupiter. Since Galileo’s time, lenses have been used in many instruments, such as microscopes and camera ...
New Planet Definition Proposed by IAU
New Planet Definition Proposed by IAU

... typically have highly inclined orbits with large eccentricities and orbital periods in excess of 200 years. We designate this category of planetary objects, of which Pluto is the prototype, as a new class that we call "plutons". (4) All non-planet objects orbiting the Sun shall be referred to collec ...
Optics - WebAssign
Optics - WebAssign

... Figure 3: Reflection and refraction of light at air-glass and glass-air boundaries When light propagates from one medium into another, the ray bends toward or away from the normal in the second medium. Which way and how much it bends depends on the optical density of the material or medium defined ...
Cones
Cones

Viewing the Universe
Viewing the Universe

... waves and microwaves. • Invisible EM radiation was discovered by Sir William Herschel using a thermometer that he placed beyond the red end of the spectrum. ...
ATNF Steering Committee – Astrophysics highlights
ATNF Steering Committee – Astrophysics highlights

... observations with the ATCA (which provided the first measurements) together with the VLA and Ryle telescopes to study the radio emission from GRB030329 which has been definitively associated with SN2003dh (Hjorth et al. Nature, 2003, 423, 847). This event is the first unambiguous link between supern ...
G030163-03 - DCC
G030163-03 - DCC

... Constraint from nucleosynthesis: ...
Lighting Information for Individuals with Cortical Vision Impairments
Lighting Information for Individuals with Cortical Vision Impairments

near-infrared adaptive optics imaging of high-redshift
near-infrared adaptive optics imaging of high-redshift

The behaviour of dark matter associated with 4 bright cluster
The behaviour of dark matter associated with 4 bright cluster

... elliptical galaxies within a core of radius 10 kpc. Such corrugation of the stellar distribution is very rare, and suggests recent formation by several simultaneous mergers. We map the distribution of associated dark matter, using new Hubble Space Telescope imaging and VLT/MUSE integral field spectr ...
Dark Matter
Dark Matter

... resulting in a tell-tale distortion of its shape. This gravitational lensing effect provides the first, and currently only, way to directly "weigh" cosmic mass. ...
Presentazione di PowerPoint
Presentazione di PowerPoint

... Beyond a few thousand Schwarzschild radii from the central SMBH, but within the sphere of influence, the motion of stars and gas is predominantly Keplerian (relativistic effects are minimal), with a component due to the combined gravitational potential of stars, dust, gas, dark matter, and anything ...
From Big Bang to Biospheres: The Scope and Limits of Explanation
From Big Bang to Biospheres: The Scope and Limits of Explanation

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Gravitational lens

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