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G-stars - Gemini Astronomie
G-stars - Gemini Astronomie

Why Study Binary Stars?
Why Study Binary Stars?

2. - Quia
2. - Quia

star a
star a

GEARS Workshop Monday - Georgia Southern University
GEARS Workshop Monday - Georgia Southern University

Assignment 8 - utoledo.edu
Assignment 8 - utoledo.edu

... a. friction, as the atoms of the expelled shell rub against each other b. the explosion of the dying star c. ultraviolet radiation from the hot star at the center d. the fusion of hydrogen into helium in the shell e. the change of electrons and protons into neutrons ____ 22. After the core of a mass ...
If you wish to a copy of this months Night Sky News
If you wish to a copy of this months Night Sky News

... prominent and brilliant star, Regulus, lying within half a degree of the ecliptic at some 85 light-years distance. In this position it is occulted occasionally by the Moon. It is a blue-white star of spectral type B7, radiating about 130 times as much light as the Sun and seen from Earth at magnitud ...
Session: [B5B-3] S3 : Stars, Exoplanets and Stellar Systems Date
Session: [B5B-3] S3 : Stars, Exoplanets and Stellar Systems Date

Shocking Truth about Massive Stars Lidia Oskinova Chandra’s First Decade of Discovery
Shocking Truth about Massive Stars Lidia Oskinova Chandra’s First Decade of Discovery

... Our analysis indicates that star may be a FAST ROTATOR V rot sin i =4000 km/s. Current mass ~10 M ...
Brock physics - Brock University
Brock physics - Brock University

17 The Deaths of Stars
17 The Deaths of Stars

... leaving stars of reduced mass called white dwarfs and remnants of expanding gases called planetary nebulae. High-mass stars die explosively as type II supernovae leaving cores of reduced mass, neutron stars or stellar black holes, and remnants of expanding gas and dust called a supernova remnants. ...
Crux The Southern Cross
Crux The Southern Cross

... locked together gravitationally to form a binary star system. Sometimes double stars may only appear close together from our vantage point on earth. If in reality they do not interact then we call this an optical double. It is possible, but rarer for 4 or 6 stars to be grouped into Computer simulati ...
(a) Because the core of heavy-mass star never reaches high enough
(a) Because the core of heavy-mass star never reaches high enough

Lec11_2D
Lec11_2D

Ch 19 Directed Reading
Ch 19 Directed Reading

... 13. top of modern H-R diagram 14. bottom of modern H-R diagram 15. right side of modern H-R diagram 16. left side of modern H-R diagram ...
answers2006_07_BC
answers2006_07_BC

... H to He in core. This stage lasts for ~90% of star’s life, which ex-6. When core He runs out, star starts fusing He plains why most stars are on MS 2. When core H exhausted, starin shell around core, becoming a giant again shrinks under gravity, heating up until H outside core starts to fuse. ...
luminosities
luminosities

... temperature (~ T4); hotter stars are brighter. ...
Lecture 17, PPT version
Lecture 17, PPT version

... All of these are stable (neither expanding nor contracting), so long as they are “left alone”. Pressure in white dwarf and neutron star is somewhat exotic (not normal gas pressure or radiation pressure) due to their highly-compressed states. ...
Lecture 9a: More on Star formation and evolution 10/22
Lecture 9a: More on Star formation and evolution 10/22

Be Stars
Be Stars

... Be stars have strong emission lines of Hydrogen in their spectrum. A characteristic of a Be star is that it has optical linear polarization and often their infra-red radiation is much greater than other B-type stars. This infra-red radiation is called infrared excess. Be stars show emission lines wh ...
Today`s Powerpoint
Today`s Powerpoint

... Energy radiated per cm2 of area on surface every second  T 4 (T = temperature at surface) And: Luminosity = (energy radiated per cm2 per sec) x (area of surface in cm2) So: Luminosity  (temperature) 4 x (surface area) Determine luminosity from apparent brightness and distance, determine temperatur ...
Stars - Mrs. Tosh`s class
Stars - Mrs. Tosh`s class

... The entire sky is lit up for weeks. The temperature can be more than 100 billion degrees. The iron atoms fuse into uranium. ...
Photosphere
Photosphere

... Sirius A is slightly larger than the sun. Sirius B is 100 1 times smaller. The same size as the Earth! Stars come in 3 sizes. Luminosity (Lsun) Î ...
Star Evolution
Star Evolution

Brock physics - Brock University
Brock physics - Brock University

... 10. The protostar phase of a star’s life is (a) * shorter for higher mass stars. (b) longer for higher mass stars. (c) [It depends on the size of the molecules comprising the star.] (d) [It depends on the whims of the head office of ProtoStar Inc.] 11. A brown dwarf is (a) a character in the Disney ...
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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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