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Navigation: The Mariner`s Quadrant
Navigation: The Mariner`s Quadrant

High precision effective temperatures for 181 F-
High precision effective temperatures for 181 F-

... The use of ∼70–100 calibrations reduces the uncertainty to 5–7 K (for spectra with S/N =100–150). Better quality spectra (R >100,000, S/N > 400) should in principle allow the uncertainty of just 1–2 K. Clearly, time variation of the temperature for a given star should be readily detected by this met ...
Homework Assignment 6 — Solutions
Homework Assignment 6 — Solutions

... Very little calcium is doubly ionized in the Sun’s photosphere; instead, the calcium is almost all in the singly-ionized state—Example 8.1.5 shows that the ratio of singly-ionized calcium to neutral calcium is very high, and that almost all of the singly-ionized calcium is in the ground state. This ...
PDF format
PDF format

CH14.AST1001.S15.EDS
CH14.AST1001.S15.EDS

... • Nothing can escape from within the event horizon because nothing can go faster than light. • No escape means there is no more contact with something that falls in. It increases the hole's mass, changes its spin or charge, but otherwise loses its identity. ...
The Sun Section 1 The Sun`s Energy, continued
The Sun Section 1 The Sun`s Energy, continued

... • Careful studies of motions on the sun’s surface have supplied more detail about what is happening inside the sun. The parts of the sun include *. • At the center of the sun is the core. The core makes up 25% of the sun’s total diameter of 1,390,000 km. The temperature of the core is about 15,000,0 ...
Properties of Wolf-Rayet Stars - Paul Crowther, University of Sheffield
Properties of Wolf-Rayet Stars - Paul Crowther, University of Sheffield

... stars, and WN6 stars either early or late-type. Complications arise for WN stars with intrinsically weak emission lines. For example, HD 93131 (WN6ha) has a He ii λ4686 emission equivalent width which is an order of magnitude smaller than that observed in other WN6 stars; the ‘ha’ nomenclature indic ...
Sample pages 1 PDF
Sample pages 1 PDF

... An attentive observer will soon notice that individual bright stars that are rather close together in the sky seem to form simple geometric shapes – squares, rhombuses, crosses, circles, arches. Giving a name to these shapes in the sky makes them more familiar to you and easier to locate again. That ...
Full Starlight Report
Full Starlight Report

... On the day you were born, you not only gained the magic of your horoscope, you also gained the myths and meanings of a sky full of stars. Not all the stars, just those that formed links to your natal planets via what is called parans. By considering the star parans in your life you will be encounter ...
The plane of the Moon`s orbit has an inclination of 5.15 degree to
The plane of the Moon`s orbit has an inclination of 5.15 degree to

... Mahabharata, the nakshatras were recognized by their Yogataras (or principal stars) which were seen within a group of other stars surrounding each of them in a recognizable form or shape in the sky. Krittika nakshatra is also recognized by the star Krittika (Aclyone 2) whose longitude is about 360 8 ...
Historic mass loss from the RS Ophiuchi system
Historic mass loss from the RS Ophiuchi system

... Stars with an initial mass between ∼ 1 and ∼ 40 M¯ become hydrogen/heliumshell-burning Asymptotic Giant Branch (AGB) stars or core-helium-burning red supergiants (RSG). These phases are characterised by cool, molecular atmospheres giving rise to M spectral types (S or C for some chemically peculiar ...
21_Testbank
21_Testbank

... C) Galaxies were closer together in the past because the universe was smaller. D) Galaxies attracted each other more strongly in the past because they were more massive; they had not yet turned most of their mass into stars and light. E) Galaxy collisions shouldn't have been more common in the past ...
The white dwarf population within 40 pc of the Sun
The white dwarf population within 40 pc of the Sun

... For each of the synthetic white dwarf populations described below, we generated 50 independent Monte Carlo simulations employing different initial seeds. Furthermore, for each of these Monte Carlo realizations, we increased the number of simulated Monte Carlo realizations to 104 using bootstrap tech ...
Molecular Gas in Galactic Environments Abstracts (Poster)
Molecular Gas in Galactic Environments Abstracts (Poster)

... Early-Type Galaxies (ETGs) have been long-classified as the red, ellipsoidal branch of the classic Hubble tuning fork diagram of galactic structure. In part with this classification, ETGs are thought to be molecular and atomic gas-poor with little to no recent star formation. However, recent efforts ...
X-ray Astronomy and the search for Black Holes
X-ray Astronomy and the search for Black Holes

... • Swift XRT has problems with CH Cyg because it is extremely bright in the optical • The other three can be fitted with a bremsstrahlung continuum plus a single Gaussian near 6.5 keV, with a strong partial covering absorber. – Note BAT spectrum is average over 9 months, XRT data are from ...
Mathematics in Art and Architecture GEM1518K
Mathematics in Art and Architecture GEM1518K

... model and the way things really are. Why a sphere? The Earth is spherical! This was known much earlier than Columbus' time. Sailors had long known that as a ship sailed away from the shore it not only diminished in apparent size, but it also appeared to sink into the water. The simplest explanation ...
Specification Topic 1 – Earth, Moon and Sun 1.1 Planet Earth
Specification Topic 1 – Earth, Moon and Sun 1.1 Planet Earth

... 3.2l explain the apparent east-west motion of the night sky 3.2m recall that stars cross the observer’s meridian and culminate when they are due south 3.2n use star data and charts to determine the time at which a star will cross the observer’s meridia n 3.3 Physical Properties of Stars Candidates s ...


... 28.8 d according to Tremko (1964). With an analysis of more than 1100 photometric observations, Mendes de Oliveira & Nemec (1988) concluded that RU Psc is not a double mode or RRd star but that the peculiarities seen in the photometry of RU Psc are due primarily to rapid and irregular period changes ...
Galaxy Spiral Arms
Galaxy Spiral Arms

... mass such as the Sun. Our Milky Way Galaxy has distributed mass, where hundreds of billions of individual stars all contribute to the total mass of the Galaxy. On a gross scale, that mass is relatively symmetrical, so for our gravitational effect on any other galaxy, yes, our entire Galaxy acts as t ...
THE N/O RATIO IN EARLY B-TYPE MAIN SEQUENCE STARS AS
THE N/O RATIO IN EARLY B-TYPE MAIN SEQUENCE STARS AS

... insensitive to overionization of the NII and OII ions. On the other hand, the N/C and C/O ratios, which include carbon, may contain systematic errors for stars with Teff > 18500 K because of neglected overionization of CII ions. The ratio N/O is studied in the atmospheres of 46 early main-sequence B ...
celestial navigation heaven`s guide for mere
celestial navigation heaven`s guide for mere

... largest known type of star and can rarely be found. When supergiant stars die, they undergo a supernova explosion and become black holes. Besides that, under the faint and virtually dead stars group, there are four other sub-groups namely white dwarfs, brown dwarfs, neutron stars and pulsars. A whi ...
POISE AND EVOLUTION OF THE GALAXY : STRUCTURE ,
POISE AND EVOLUTION OF THE GALAXY : STRUCTURE ,

... Furthermore, some so-called “black holes” are similarly regarded as intensely radiating sources (just like “WHITE WELLS”), through various arguments : we might, more naturally, connect them to some cosmic regions of matter and antimatter, possibly undergoing gravitational attraction, at first, and e ...
Babylonian Capricorn
Babylonian Capricorn

... thus constantly interacting with the sun, moon and planets, it has surprisingly little lore directly associated with it in either Babylonian or Greek traditions. Consequently, if we want to describe the symbolic nature of the constellation, we have to fall back on other, more indirect methods. The f ...
astro-ph/9410035 PDF
astro-ph/9410035 PDF

... comparable rates in both regions, and most of the heat generation and energy emission (in the form of neutrinos) occurs in the outer region. Gnedin and Yakovlev (1994) have proposed that a temperature gradient in the core of a neutron star may generate convective motions that would further complicat ...
Parent stars of extrasolar planets III: ρ1 Cancri Revisited
Parent stars of extrasolar planets III: ρ1 Cancri Revisited

< 1 ... 31 32 33 34 35 36 37 38 39 ... 433 >

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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