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PowerPoint 프레젠테이션
PowerPoint 프레젠테이션

... Observations of NS-MS(main sequence) binary requires different evolution process ...
October 2014 - Newbury Astronomical Society
October 2014 - Newbury Astronomical Society

... in the true sense of the word, its aging process does allow us to use some of the terms that we use to describe the aging process of living things. Stars are created (born), they do get older of course and they do eventually stop shining and in effect die. Stars are born in Stellar Nurseries within ...
Journey to the Stars Educator`s Guide
Journey to the Stars Educator`s Guide

... nuclear fusion occurs, producing energy. The outward pressure of gas heated by fusion is balanced by the inward pull of gravity, leaving the star in hydrostatic equilibrium. This balance of forces lasts for most of a star’s life, maintaining its steady temperature. Radiation and convection carry the ...
Stars - CBSD.org
Stars - CBSD.org

... to undergo fusion at the core. • Without enough “accretion,” however, fusion may never start. – The mass never becomes luminous, instead turning into a brown dwarf. – Despite the name, brown dwarfs are still 15-75x the mass of Jupiter. • They’re named for being “dark.” ...
Synthetic Stellar Populations Encyclopedia of Astronomy & Astrophysics eaa.iop.org Guy Worthey
Synthetic Stellar Populations Encyclopedia of Astronomy & Astrophysics eaa.iop.org Guy Worthey

... a billion years of age. This is because almost all the light comes from stars near the main sequence turnoff or from post-main-sequence stars. All of these stars have nearly the same mass (because post-main-sequence lifetimes are relatively short) so there is little mass differential for the IMF to ...
Astronomy - SparkNotes
Astronomy - SparkNotes

... Atmosphere: The balance between the force of gravity on a planet and its average surface temperature determines the amount and composition of its atmosphere. • If the average velocity of gas molecules (determined by surface temperature) is greater than the escape speed of the planet (determined from ...
Stars and Planets - The University of Texas at Dallas
Stars and Planets - The University of Texas at Dallas

... The Pleiades is a famous cluster of young stars visible in the constellation Taurus. When most of the gas and dust is gone from a stellar nursery, the young stars are in an open cluster. One day these star systems will drift apart. Image source: http://antwrp.gsfc.nasa.gov/apod/ap021201.html ...
Requests from our TA (and me)
Requests from our TA (and me)

... The Earth orbits around the Sun with a speed of 30 km/s. The speed of light is 300,000 km/s. I observe infrared radiation from sulfur atoms which is emitted at a wavelength of 10 µm. What is the difference between the emitted wavelength and the wavelength I observe from the moving Earth? A. .001 µm ...
Lecture 6 - Stars and Distances
Lecture 6 - Stars and Distances

HIGH RESOLTION SPH SIMULATIONS OF GALAXY CLUSTERS
HIGH RESOLTION SPH SIMULATIONS OF GALAXY CLUSTERS

... be formed at high redshift ...
PPV_hd169142
PPV_hd169142

... law, indicative of dust settling. The presence of extended PAH emission is expected in such a comparatively flat disk if there is a central cavity in the disk. The presence of a cavity is supported by the low level of the UV excess light, the weak Mg II and H emission and the absence of a high velo ...
FIRST LIGHT IN THE UNIVERSE
FIRST LIGHT IN THE UNIVERSE

... galaxies from 3
Stars
Stars

... • THE SUN! • The sun is a medium sized star • MUCH, MUCH larger than Earth ...
MS Word version
MS Word version

... demonstrating the Eclipsing Binary Simulator in a classroom situation. We provide these suggestions with appropriate questions (shown in bold italics) to pose to the class as an aid in promoting interactivity. We encourage instructors to adapt these suggestions to their particular educational goals ...
Document
Document

...  A star is born when temperature and pressure at its center become great enough to start nuclear fusion. ...
Document
Document

... • Brightness: distance and energy output - Luminosity – total energy emitted by a star ...
NGC 3370 Spiral Galaxy - University of Kentucky
NGC 3370 Spiral Galaxy - University of Kentucky

... NGC 4526, distance ~ 200 million light years. ...
Effects of r-modes induced differential rotation on long-term
Effects of r-modes induced differential rotation on long-term

... A and N are two constants determined by the initial condition. Sa & Tome (2005) suggested N = 2l -1 and redefined A by introducing a new free parameter K as This second-order solution gives a differential ...
Measuring the Distance to Stars Using Parallax
Measuring the Distance to Stars Using Parallax

Document
Document

... Estimate the intensity of the radiation emitted per unit area from a star if it’s effective surface Temp is 6000K Estimate the energy emitted from a star if its peak wavelength is 600nm. Total power radiated Power output = E x surface area of star Surface area of a star = 4  R 2 Where R is the rad ...
GRAVITATIONAL RADIATION FROM ACCRETING NEUTRON STARS
GRAVITATIONAL RADIATION FROM ACCRETING NEUTRON STARS

... obviously in X-ray binary systems, and some of these are potential strong gravitational wave sources [4]. But accretion occurs in other situations, most notably in Thorne-Zytkow objects, which are the stage of evolution of massive X-ray binaries that occurs after the X-ray phase, when the giant comp ...
NS-BH
NS-BH

The Solar System and our Universe
The Solar System and our Universe

... about the origin of the Universe? (M5 & M6) • Scientists believe that the red shift evidence tells us that at some point in time, billions of years ago, all the mater & energy in the Universe was concentrated in the same place. • A massive explosion tool place – Big Bang. • It flung all the matter & ...
Project Packet - Montville.net
Project Packet - Montville.net

... What’s Your Sign? Constellations, Stars and the Hertzsprung-Russell Diagram ...
The Observer Newsletter - the TriState Astronomers
The Observer Newsletter - the TriState Astronomers

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Star formation



Star formation is the process by which dense regions within molecular clouds in interstellar space, sometimes referred to as ""stellar nurseries"" or ""star-forming regions"", collapse to form stars. As a branch of astronomy, star formation includes the study of the interstellar medium (ISM) and giant molecular clouds (GMC) as precursors to the star formation process, and the study of protostars and young stellar objects as its immediate products. It is closely related to planet formation, another branch of astronomy. Star formation theory, as well as accounting for the formation of a single star, must also account for the statistics of binary stars and the initial mass function.In June 2015, astronomers reported evidence for Population III stars in the Cosmos Redshift 7 galaxy at z = 6.60. Such stars are likely to have existed in the very early universe (i.e., at high redshift), and may have started the production of chemical elements heavier than hydrogen that are needed for the later formation of planets and life as we know it.
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