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AST1100 Lecture Notes
AST1100 Lecture Notes

... Most models of star formation tell us that the formation of planets is a common process. We expect most stars to have planets orbiting them. Why then, has only a very few planets (less than ten by fall 2009) around other stars been seen directly? There are two main reasons for this: 1. The planet’s ...
Document
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... a center 100-150 pc from the Sun Inclined respect to the ...
Using Star Charts
Using Star Charts

... Getting to know the Heavens, and the motions of Sun, Moon and Stars If the sky is imagined to be a celestial sphere, then the stars may be represented on a map in much the same way that the spherical Earth can be mapped onto a flat piece of paper. The lines of latitude and longitude on a map of the ...
Abundances of RGB stars in NGC 6752 Grundahl
Abundances of RGB stars in NGC 6752 Grundahl

SWA (Sliding Window Algorithm) V1.0 User·s Guide
SWA (Sliding Window Algorithm) V1.0 User·s Guide

... without aberration. The precision should be worth with the real PSF, but it depends on the correction used that has not been tested yet ; Magnitude precision is 0.15 mag. at 20 magnitude, and 0.3 mag. at 21. A bias can be observed from magnitude 20.5, just because it is under the detection limit : s ...
Li-cai Deng
Li-cai Deng

... of one galaxy instead of comparing snapshots of many. It is only now that we have large surveys of the whole sky that we are able to comprehend the Milky Way as a whole. Unlike external galaxies, the picture we are building is in three dimensions of position and velocity, with much higher accuracy i ...
Stellar Magnetic Activity
Stellar Magnetic Activity

... RS Cvn binary systems ...
Essential Question
Essential Question

... 6. If a star has a low surface temperature and is considered very dim, where would you expect it to be located on the Herztsprung-Russell diagram? ...
18_Testbank - Lick Observatory
18_Testbank - Lick Observatory

... A) The entire mass of Earth would end up as a thin layer, about 1 cm thick, over the surface of the neutron star. B) It would rapidly sink to the center of Earth. C) The combined mass of Earth and the neutron star would cause the neutron star to collapse into a black hole. D) It would crash through ...
b. - UW Canvas
b. - UW Canvas

... dependence of the parallax angle on the distance an object is from Earth. If the minimum parallax angle we could measure were 0.5 arcsec, what is the maximum distance of a star that we could measure? ...
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... Studying radio waves emitted by objects in space gives astronomers data that are not available from the visible spectrum. Radio waves are received from stars, galaxies, nebulae, black holes, and even some planets—both in our own solar system and in others. These signals are mapped through the use of ...
Chapter 10 Neutron Stars and General Relativity
Chapter 10 Neutron Stars and General Relativity

... pulsar and is clock-like in its precision. Thus • Variations in that period as observed from Earth must be associated with orbital motion in the binary. • These variations can be used to give very precise information about the orbit. • When the pulsar is moving toward us, the repetition rate of the ...
cohen_paris_v2_may2009 - Astronomy at Swarthmore College
cohen_paris_v2_may2009 - Astronomy at Swarthmore College

... narrower lines and rotationally modulated variability, in general agreement with MHD simulations. Line ratio diagnostics are useful for localizing the hot plasma, and indicate that the MHD simulations predict a location that is too far from the photosphere. ...
April 2016 - Newbury Astronomical Society
April 2016 - Newbury Astronomical Society

... Earth we need to go back in time to think about how Earth and the Moon formed. Evidence suggests that in the early solar system there were many more planets than the eight we have today. There may have been 30 or more and possibly as many as 80 when the Solar System formed. Many of these fledgling p ...
Abstract - UChicago High Energy Physics
Abstract - UChicago High Energy Physics

... composition [2, 9, 12–16]. The neutrino flavor composition above the neutrino trapping surface depends not only on thermodynamics in the trapped regions, but also the oscillation of neutrinos as they leave the disk. The high neutrino density coupled with high matter density provide an environment wh ...
Starfarer
Starfarer

... is seen to arch towards the north. Firth (1954) states that the star path from Tikopia to Anuta (54 deg) has nine stars, whereas for the passage from Ninigo to Kaniet ( dir 80 deg, much east) only 5 stars are needed. ( Statement by Itilon of Amich, Ninigo, 1969) Hence each voyage vary in the number ...
NGC 1808 - Rencontres de Moriond
NGC 1808 - Rencontres de Moriond

... by the active source: + The contribution to soft X-rays might be non-negligible, but is is any case below 30%. + The contribution to hard X-rays is negligible. + The SSC could produce only around 1/50 of the ionizing photons producing the observed emission line spectrum, and no more than 1/10 of the ...
ppt
ppt

... million years. Disturbance shifts the orbits of many distant comets, making them plunge into the inner solar system. A small number of those comets hit the Earth, causing the mass extinctions. ...
Galaxy Formation and Evolution
Galaxy Formation and Evolution

... Any hot gas associated with the progenitors is shock-heated during the merger and settles back into hydrostatic equilibrium in the new halo. If the progenitor halos contained central galaxies, the galaxies also merge as part of the violent relaxation process, producing a new central galaxy in the fi ...
01 - MrPetersenScience
01 - MrPetersenScience

... _____ 64. To what does the word atmosphere refer when applied to the sun? a. the sheath of air surrounding the sun b. all the gases that make up the sun c. the uppermost region of solar gases d. the regions of gases above the sun’s core _____ 65. What are the three layers of the sun’s atmosphere? a. ...
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flare swg usa

... resolution, near-IR fluxes from clustered sources are often very much fainter. FLARE can reach ~8 mag deeper than IRAC surveys at 3.5 μm, enabling the measurement of the NIR SEDs of young (<104 yr old) protostellar sources. CfA currently is extending the Robitaille YSO grid code with the abil ...
Chemical Evolution
Chemical Evolution

... Predictions for disk galaxies:  Extended disks form late, after most merging complete, or redshift ~ unity (~8Gyr ago) (mass-dependent, 1012M)  Hundreds of satellite dark haloes  Stellar halo formed from disrupted satellites  Minor mergers (< 20% mass of disk ) heat thin disk, create thick dis ...
Latitude and Longitude - Harvard University Laboratory for
Latitude and Longitude - Harvard University Laboratory for

... Fraction of day since midnight ...
Celestial Equator
Celestial Equator

... • Note that right ascension is measured eastwardly along the equator, starting at the vernal equinox. • Note that 24h is the same as 0h. • Hours of right ascension are subdivided into minutes and seconds. However, these are not equivalent to the minute and second subdivisions of degrees of declinati ...
Educator`s Guide to the Cullman Hall of the Universe, Heilbrunn
Educator`s Guide to the Cullman Hall of the Universe, Heilbrunn

... of gravity and electromagnetism. At the same time, galaxies are colliding: smaller galaxies and surrounding gas merged to form the Milky Way, which is now on a collision course with the Andromeda Galaxy. All stars (including our Sun) are born, shine until they run out of fuel, and die. The most mass ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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