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The HERMES GALAH survey: overview
The HERMES GALAH survey: overview

... Galactic bar or spiral structure. The Hercules group seen in Figure 3 is an example. Its stars are chemically a typical sample of the nearby disk, with a wide range of chemical abundances. These resonance groups are dynamically interesting but are of limited interest for Galactic archaeology. Some ...
CELESTIAL MANUAL:CELESTIAL MANUAL
CELESTIAL MANUAL:CELESTIAL MANUAL

Part IV: Stars
Part IV: Stars

... Instructor Guide for The Essential Cosmic Perspective, Sixth Edition 140 Sun is yellow, they can have trouble with the idea that the Sun would look nearly white if they were not seeing it through Earth’s atmosphere. However, when astronomers speak of “white stars,” they are usually talking about st ...
Stars - Emera Astronomy Center
Stars - Emera Astronomy Center

17_Testbank
17_Testbank

... A) The giant must once have been the more massive star but transferred some of its mass to its companion. B) Despite the low odds of finding a system with two such massive stars, there is nothing surprising about the fact that such systems exist. C) The two stars probably were once separate but beca ...


... 3. THE RR LYRAE STARS IN M15 In Clement’s (2002) data base of variables stars, a total of 158 variable stars are known, from which approximately 104 are RR Lyrae type stars. In this work, 33 known RR Lyrae stars, identified in Figs. 1 and 2 and listed in Table 4, have been studied. For all the stars ...
Observing Stellar Evolution
Observing Stellar Evolution

White dwarf binaries
White dwarf binaries

... Flickering found in UX UMa (Linnell 1949, 1950) 71 s pulsations in DQ Her (Walker 1956) Identification of WD as primary in CVs AE Aqr secondary filling Roche lobe (Crawford and Kraft 1956) All CVs are binaries undergoing mass transfer onto WD (Kraft 1962) Accretion disk responsible for outburst ligh ...
black hole
black hole

...  The first white dwarf discovered was the faint companion to the well-known star Sirius.  Sirius, the brightest star in the sky, is a visual binary star, the most luminous member of which is Sirius A.  The white dwarf, Sirius B, is 10,000 times fainter than Sirius A. ...
StellarManual
StellarManual

... An incomplete sentence is presented that indicates the size and surface temperature a certain star has relative to the Sun. Students should determine how the stellar luminosity will compare with the Sun. Initially there is no equation displayed. Answer: Luminosity of a star is proportional to the sq ...
Polaris
Polaris

... While being honored as the North Star, Polaris enjoys the title of Lodestar and Cynosure as well. Polaris science. The single point of light that we see as Polaris is actually a triple star system, or three stars orbiting a common center of mass. The primary star, Polaris A, is a supergiant with abo ...
Lecture 14
Lecture 14

... Alternative unit of distance “1 Light Year is the distance traveled by light in one year.” Relation to other units: 1 light year (ly) is equivalent to 0.31 pc 63,270 AU ...
151 - ESO
151 - ESO

WHAT MAKES A STAR SO SPECIAL Abstract
WHAT MAKES A STAR SO SPECIAL Abstract

... 1. The teacher introduces the physical characteristics of stars and the spectral classification to the students (you can use the information from the Introduction section as a supplement to the lesson about Star characteristics in the textbook you are using). 2. The teacher gives every student an en ...
Teacher`s Guide - Cornell Science Inquiry Partnerships
Teacher`s Guide - Cornell Science Inquiry Partnerships

... Astronomy, Earth Science Audience This activity is aimed at a high school audience, but it could easily be modified for use with middle school students. Time Required The essential activities can be covered in 40 minutes, or the entire project can be stretched to 4 hours or even much longer. (In the ...
Common Envelope Evolution Leading to Supernovae with Dense
Common Envelope Evolution Leading to Supernovae with Dense

Star Formation in Bok Globules - European Southern Observatory
Star Formation in Bok Globules - European Southern Observatory

... is a huge, faintly luminous H 1I region spread over more than 30 degrees of the southern sky. At a distance of roughly 450 pc this corresponds to a radius of about 125 pc, making the Gum Nebula one of the largest structures known in our galaxy. Near its center are several objects which tagether prod ...
Searching for RR Lyrae Stars in M15
Searching for RR Lyrae Stars in M15

the UKIRT Fundamental and Extended lists
the UKIRT Fundamental and Extended lists

JHK standard stars for large telescopes: the UKIRT Fundamental
JHK standard stars for large telescopes: the UKIRT Fundamental

... capacitance. The observations were done through apertures of angular diameter 8 or 12 arcsec on the sky, with background removal by chopping with the secondary mirror. The observations were made relative to numerous stars from the CIT-based UKIRT ‘in-house’ standards, mentioned above. The results we ...
Devil physics The baddest class on campus IB Physics
Devil physics The baddest class on campus IB Physics

Cepheid
Cepheid

... That They Were All Identical …then life becomes very simple! Suppose, for example, that Henrietta later found a Cepheid in a more remote nebula (like M31, the Andromeda nebula) It would look much fainter than the ones she has been observing in the nearby LMC. This tells us the relative distance. [Fo ...
Stellar Masses
Stellar Masses

... called brown dwarfs, and are ‘star like’ in the sense that nuclear burning of deuterium occurs in their core. Below a mass of 0.015M⊙ (roughly 16 times the mass of Jupiter) not even deuterium burning can occur, and these objects are perhaps best called planets. Thus there is a natural lower limit to ...
A very massive runaway star from Cygnus OB2⋆
A very massive runaway star from Cygnus OB2⋆

... system is 58 84, very similar to the position angle of its resid- ...
On the nature and detectability of Type Ib/c supernova progenitors
On the nature and detectability of Type Ib/c supernova progenitors

< 1 ... 5 6 7 8 9 10 11 12 13 ... 132 >

Corona Borealis

Corona Borealis /kɵˈroʊnə bɒriˈælɨs/ is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means ""northern crown"". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern. The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from our Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.
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