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Westerlund 1 : A Super-Star Cluster within the Milky Way
Westerlund 1 : A Super-Star Cluster within the Milky Way

... presence of several yellow hypergiants (Westerlund 1987) hint that Wd1 could represent a very massive cluster, since such stars represent only a short phase in the evolution of massive stars. ...
r 0
r 0

... 3 arcsec = 1.45e-5 rd =lvis/r0 : r0(0.5µm)=3.4cm sf2=1.03(D/r0)5/3 = 283 rd2 at lvis=0.5µm sf2(0.5µm) 0.52 = sf2(10µm) 102 => sf2(10µm) = 0.71 rd2 SR = exp(-0.71) = 0.49 ...
Exercise 8
Exercise 8

... How accurate were you? Is the criterion or criteria you used a good way to find galaxy distances? ...
ph507rev1
ph507rev1

... Technological advances (including the Hubble Space Telescope) have improved parallax accuracy to 0.001” within a few years. Before 1990, fewer than 10,000 stellar parallaxes had been measured (and only 500 known well), but there are about 1012 stars in our Galaxy. Space observations made by the Euro ...
Stars - CBSD.org
Stars - CBSD.org

... – That’s a telescope filter, designed to cut down on light pollution (brightening of the skies due to electric light at night). – The filter is advertised as blocking light from fluorescent or incandescent sources but still letting the light from galaxies and nebulae through. ...
Economic Feasibility of a Siderostat-fed Liquid Mirror Telescope for
Economic Feasibility of a Siderostat-fed Liquid Mirror Telescope for

... field of view (arcminutes or less) to be observed at fixed zenith angles up to 45 degrees [13], but this solution is cumbersome and - since it is limited to a single angle - seemingly not practical. A design that allows pointing within a limited field of regard (˜ 6 degrees diameter) centered on the ze ...
The Dynamics of the Galaxies in the Local Group
The Dynamics of the Galaxies in the Local Group

... – It may even hit the Milky Way first (9% probability) … – … or it could escape from the Local Group (7% probability) ...
What Is A Spectrum?
What Is A Spectrum?

... Fraunhofer (1787-1826) looked at sunlight with an even better prism and saw 600 such dark lines in the spectrum. Finally, Gustav Kirchhoff (1824-1887) figured out what was going on and gave the world a set of rules describing what was making both the continuous spectrum that Newton saw and the dark ...
G020297-00 - DCC
G020297-00 - DCC

... Einstein theorized that smaller masses travel toward larger masses, not because they are "attracted" by a mysterious force, but because the smaller objects travel through space that is warped by the larger object LIGO-G020297-00-M ...
Spectroscopy: Unlocking the Secrets of Star Light
Spectroscopy: Unlocking the Secrets of Star Light

... sodium or neon) at rest with respect to the spectrograph, allowing the spectrum of the distant source to be calibrated and any shift of spectral lines to be measured. Recording the Spectrum Newton recorded the spectrum of sunlight by drawing it. The rise of spectroscopy for astronomical use was in p ...
Here
Here

... the x-axis of the plot, and some measure of the intrinsic luminosity is plotted on the y-axis. ...
Spectroscopy: Unlocking the Secrets of Star Light
Spectroscopy: Unlocking the Secrets of Star Light

... sodium or neon) at rest with respect to the spectrograph, allowing the spectrum of the distant source to be calibrated and any shift of spectral lines to be measured. Recording the Spectrum Newton recorded the spectrum of sunlight by drawing it. The rise of spectroscopy for astronomical use was in p ...
Scientific Justification
Scientific Justification

... amount of time. All objects were examined visually using the SPOT imaging tools to verify that bright objects do not fall in regions which could scatter light into the IRAC field of view. IRS Staring Observations - We request a total of 21.76 hours using all four SL and LL modules of IRS in staring ...
hanson.pdf
hanson.pdf

Primary and secondary eclipse spectroscopy with JWST: exploring
Primary and secondary eclipse spectroscopy with JWST: exploring

... or ices, of non-solar composition. This volatile content represents a small fraction of the total planetary mass and is fractionated between the interior (crust, mantle), the surface oceans and/or ice sheets, the atmosphere and outer space through gravitational escape (induced by impacts, exospheric ...
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... before fading from view after nearly two years. •Even today, the nebula • is still expanding at • more than 3 million ...
z - STScI
z - STScI

... across the inner hole ...
SACE 2 Physics Key Ideas Textbook Third Edition Part 2 sample
SACE 2 Physics Key Ideas Textbook Third Edition Part 2 sample

... Because the satellite is positioned above the equator, when viewing regions near the equator from a geostationary satellite, we are viewing the surface of the Earth at an angle of 90“ to the surface. Because of the curvature of the Earth’s surface, when looking at high latitudes from a geostationary ...
Midterm Exam, AST 203, Spring 2012 Thursday, March 15, 3:00
Midterm Exam, AST 203, Spring 2012 Thursday, March 15, 3:00

... in numbers for the luminosity of the Sun and σ. As above, 7 points for writing down the relation between L, T, and r, and 7 more points for realizing that the way to go is to take a ratio. 2. Two Planets (70 points) Consider two planets in circular orbits around a main sequence B star. The star has ...
"Magnetic Field Structure in Relativistic Jets", H. Jermak
"Magnetic Field Structure in Relativistic Jets", H. Jermak

... been observed by gamma-ray telescopes can give insight into magnetic field structure in the jet by comparison with model predictions. GRB 060418 = no large-scale ordered magnetic field? GRB 090102 = largescale ordered magnetic field? Cannot rule out possibility that each GRB outflow has very diffe ...
Pluto Challenge - Cedar Amateur Astronomers
Pluto Challenge - Cedar Amateur Astronomers

... of Pluto’s discovery in a book titled “The Search for Planet X”. I don’t remember the author but I’ve always remembered the tale of Clyde Tombaugh’s tireless search for the suspected “Planet X”. It wasn’t until Tombaugh’s discovery on January 23, 1930 that our view of the solar system grew from eigh ...
I. The Spectrometer and the Balmer Series
I. The Spectrometer and the Balmer Series

... the Balmer spectrum. Determine R, and the uncertainty of R, by fitting your data to a linear plot. Discuss the uncertainty of the fit and the uncertainty of your measurements. The given value of R is found in your text or the Handbook. The values for the lines may be readily calculated from R and th ...
every star in the cluster.
every star in the cluster.

... giants, continually forming from evolving stars near the turnoff. But there were originally many stars that were even more massive, that became red giants for a time, and that have moved on to a different final form. The cluster contains a huge number of ‘stellar remnants.’ [Details to follow!] ...
chapter16StarBirth
chapter16StarBirth

... sort of force stops contraction before the core temperature rises above 107 K. • Thermal pressure cannot stop contraction because the star is constantly losing thermal energy from its ...
Galileo`s miraculous year: 1609 and the revolutionary telescope
Galileo`s miraculous year: 1609 and the revolutionary telescope

... assumed to be at varying distances from the Earth, should discovery, because its orbital period is 165 years. The first exhibit parallax as the Earth changes position in its orbit over orbit will be completed in 2011. the course of a year. Galileo was well aware of this feature of the heliocentric mo ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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