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Document
Document

... Gray reported bisector variations of 51 Peg with the same period as the planet. Gray & ...
Gemini - www.BahaiStudies.net
Gemini - www.BahaiStudies.net

... To look at Gemini is to look away from the Milky Way; as a result, there are comparatively few deep-sky objects of note. The Eskimo Nebula and Medusa Nebula, Messier object M35, and Geminga are those that attract the most attention. The Eskimo and Medusa nebulae are both planetary nebulae, the one a ...
Measuring Starlight Deflection during the 2017 Eclipse: Repeating
Measuring Starlight Deflection during the 2017 Eclipse: Repeating

... night will give a good starting point, changes in temperature will require a small adjustment, especially since the depth of focus for the Tele Vue NP101is is only about ± 2*λ*(focal ratio)2, or ± 37 microns for red light. Fortunately, the focuser can easily achieve this resolution using its 10:1 fi ...
CVs
CVs

... • Usually only off by ~1% • Possibly knocked out of synchronous rotation – V1500Cyg Nova ...
iStage2_EN_iSky smart measurements of the heaven
iStage2_EN_iSky smart measurements of the heaven

... Throughout history, the use of the stars has been an important tool for determining the position of individuals and places on the Earth. From the viewpoint of European history, the astrolabe could be considered the first mechanism that was used to locate a star in space. During the great voyages in t ...
Document
Document

... • At least four supernovae have been observed in our Milky Way galaxy during the last thousand years, in ...
Lectures 14 & 15 powerpoint (neutron stars & black holes)
Lectures 14 & 15 powerpoint (neutron stars & black holes)

... the companion star, forming an accretion disk. Heats up to a few million K. => Strong X-ray source! ...
Multi-physics simulations using a hierarchical interchangeable
Multi-physics simulations using a hierarchical interchangeable

... combined to conduct numerical experiments. The community codes are generally written independently, so AMUSE encompasses a wide variety of computer languages and programming styles. The fundamental design feature of the framework is the abstraction of the functionality of individual community codes ...
26.9 news and views feature mx
26.9 news and views feature mx

... Natural philosophers have speculated on the existence of worlds around other suns for millennia. Now that real data are available, we find a diversity far beyond that expected by scientists, or science-fiction writers. n the 1960s, with great fanfare, the discovery of first one, and then two Jupiter ...
Astronomical Formulae
Astronomical Formulae

... Where D is the diameter of the objective in inches Atmospheric conditions seldom permit Theta > 0.5". The Dawes Limit is one half the angular diameter of the Airy (diffraction) disc, so that the edge of one disc does not extend beyond the center of the other). The working value is two times the Dawe ...
Galaxies * Island universes
Galaxies * Island universes

... Galaxies formed by gravitational infall of proto-galactic clumps which were already forming stars by the time they came together, forming spheroid, and bulge Disk formed from later infalling gas of higher angular momentum, which dissipates against itself to settle into a thin disk A Galaxy’s color e ...
Light and Spectroscopy Concept Inventory
Light and Spectroscopy Concept Inventory

... marked in the drawing. By comparing the positions of the lines in the spectrum to a known laboratory spectrum on Earth, which of the following properties of the nebula can be directly determined? a. Motion towards or away from Earth only. b. Temperature only. c. Chemical composition (type of atoms) ...
N5128PNSydney
N5128PNSydney

... This strong line allows detection of PN; high [O III]/Hα ratio discriminates against H I I regions Other lines of H, He, N, Ne, Ar, S prominent in optical spectra of PN Line ratios dependent on Te, Ne and abundance Some line ratios of same species dependent on Te and/or Ne. Example: [O III]5007/4363 ...
Stars, Galaxies, and the Universe Section 1
Stars, Galaxies, and the Universe Section 1

... compact, these regions spin and shrink and begin to form a flattened disk. The disk has a central concentration of matter called a protostar. • The protostar continues to contract and increase in temperature for several million years. Eventually the gas in the region becomes so hot that its electron ...
Early Star-Forming Galaxies
Early Star-Forming Galaxies

... 9 billion to 11 billion years ago. Scientists would particularly like to know whether a quasi-steady, long-lasting process in isolated galaxies or a more rapid, starburst mode in large, merging galaxies increased the production of stars. Recent findings from a study using Hubble  and the European Sp ...
Feedback - Cambridge University Press
Feedback - Cambridge University Press

... by stars with M∗  40M ; since these stars have lifetimes ∼ 4 Myr, free-free emission traces only the most recent 4 Myr of star formation. Having found the sources of the bulk of the ionizing photons in the Milky Way, we then examined radio recombination line radial velocity catalogs to find the rad ...
Document
Document

... Stars in cluster ellipticals are old, there seems little doubt, and they also appear to be assembled into mature galaxies very early. But, cluster ellipticals are rarer than those in lower-density environments -- are these “field” ellipticals really all that different (stellar age, assembly age) fr ...
Study Guide for Earth Science Final
Study Guide for Earth Science Final

... 79. What is the shape of the planets orbits? 80. What are the different forms of electromagnetic radiation? ...
New product range (an implementation plan for business expansion)
New product range (an implementation plan for business expansion)

... This project represents a major new initiative for STAR Industries and is in many ways a new line of business. The existing management structure at STAR will be appropriate for overseeing the first part of this new project. This is due to the utilisation of existing resources with minimal new produc ...
Chapter 16
Chapter 16

... 1. The density wave theory was first proposed by Lindblad in 1960. It is a model for spiral galaxies that proposes that the arms are the result of density waves sweeping around the galaxy. 2. A density wave is a wave in which areas of high and low pressure move through the medium. 3. The density wav ...
HR Diagram Explorer Worksheet
HR Diagram Explorer Worksheet

... Open the HR Diagram Explorer. Begin by familiarizing yourself with the capabilities of the HertzsprungRussell Diagram Explorer through experimentation.  An actual HR Diagram is provided in the upper right panel with an active location indicated by a red x. This active location can be dragged around ...
The Milky Way By
The Milky Way By

... the Local Fluff inside the Local Bubble, and in the Gould Belt, at a distance of 7.62±0.32 kpc (~25,000±1,000 ly) from the Galactic Center. Padurariu Cristian & Danciu Serban ...
ppt - Faculty Virginia
ppt - Faculty Virginia

... In the Summer, the Sun is well north of the celestial equator and behaves more like a star near the north celestial pole (more like a circumpolar star) – so it is above the horizon much more than 12 hours. ...
Chapter 13 section 2
Chapter 13 section 2

... closer to Earth than other stars. Light from the Sun reaches Earth in about eight minutes. Light from other stars takes many years to reach Earth. The Sun is unusual in one way. It is not close to any other stars. Most stars are found in groups of two or more stars that orbit each other. Stars can a ...
public_lector_10
public_lector_10

... For a long time, spiral structure was thought to be a steady wave, propagating around the Galaxy. Now we think it comes and goes, as in the movie - needs gas to maintain the spiral structure and star formation. Without replenishment of the gas, the star formation and spiral structure should go out ...
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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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