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... 1999: using ASCA, X-1 in M82 was found to vary by up to a factor of four, confirming that this bright source was indeed a single object. *Over half of ULXs are known to be variable, ruling out the multiple source or SNR hypothesis. ...
Satellite Command And Data Handling Subsystem
Satellite Command And Data Handling Subsystem

... Microsatellite Case Study-MOST  The MOST (Microvariability and Oscillations of Stars) astronomy mission is Canada's first space science microsatellite and Canada's first space telescope.  Satellite's mission: to conduct long-duration stellar photometry observations in space  A secondary payload ...
A. B. C. Walker - Wisconsin Association of Physics Teachers
A. B. C. Walker - Wisconsin Association of Physics Teachers

... regions of the electromagnetic spectrum. Walker’s work involved excellent understanding of the physics of the Sun but also the use of new techniques for focusing ultraviolet radiation. Finally, he worked with a large multidisciplinary team so he also possessed considerable skill as a project manager ...
XMM-Newton observatory-I. The spacecraft and operations
XMM-Newton observatory-I. The spacecraft and operations

Angular resolution
Angular resolution

... Why the shift to southern hemisphere? ...
dtu7ech03 pt 2 - Fort Thomas Independent Schools
dtu7ech03 pt 2 - Fort Thomas Independent Schools

... visibility of celestial objects. This is called light pollution, and has been an increasing problem in recent years. The view from Kitt Peak National Observatory of the Tuscon, Arizona skyline in 1959 ...
The Ultimate Tool of Astronomy: Telescopes
The Ultimate Tool of Astronomy: Telescopes

Chapter 5 Telescope Test
Chapter 5 Telescope Test

... Chapter 5 Telescope Test Astronomy DIRECTIONS: Answer the following questions with the most complete answer. True/False: 1._____ The primary purpose of a telescope is to collect light 2._____ A Newtonian telescope has no secondary mirror 3._____ Radio telescopes are large because of the long wavelen ...
VLT identifications in the Chandra/XMM
VLT identifications in the Chandra/XMM

... sion lines and high-excitation lines indicating photoionization by a hard continuum source. However, already in the spectroscopic identifications of the ROSAT Deep Surveys it became apparent, that an increasing fraction of faint X-ray selected AGN shows a significant, sometimes dominant contribution ...
Analysis of Two Pulsating X-ray Sources
Analysis of Two Pulsating X-ray Sources

PS#3
PS#3

English version
English version

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Satellite web hunt

... Why do the satellites occupy the orbits they do? (Communications and weather satellites are usually placed in a geostationary orbit. They orbit above the Earth’s equator and have a period and direction that matches the rotation of the Earth. This allows the satellite to stay above the same point on ...
Running head: THE SUN THE SUN Physics 1040 Solar System
Running head: THE SUN THE SUN Physics 1040 Solar System

... chromosphere. [9] All of these surface features are observable due to our advances in technology and instruments which are used in observing the Sun. Missions and Observatories There are different types of solar observatories, some are located here on Earth at high elevations whereas others are in s ...
Slide 1
Slide 1

... (XRT) Swift's X-Ray Telescope (XRT) is designed to measure the fluxes, spectra, and lightcurves of GRBs and afterglows over a wide dynamic range covering more than 7 orders of magnitude in flux. The XRT can pinpoint GRBs to 5arcsec accuracy within 10 seconds of target acquisition for a typical GRB a ...
Hoffmann_Photon_Science_Novosibirsk_1__2015
Hoffmann_Photon_Science_Novosibirsk_1__2015

... As a result a new neutral and very light particle is predicted, the Axion (Weinberg, Wilczeck) Couples with two photons via Primakoff Effect in any model ...
Lecture 18, Gravitational Waves, Future Missions and
Lecture 18, Gravitational Waves, Future Missions and

... - hard X-ray sensitivity and spatial resolution - spectral resolution - all-sky survey depth ...
Slides from Dr. Frank`s Lecture17
Slides from Dr. Frank`s Lecture17

... 1) The binary separation decreases because of gravitational radiation and other angular momentum losses. 2) The component stars will evolve and change size (for example becoming a red giant) Conclusion: Long period (wide) binaries may never become interacting while short period (close) binaries are ...
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Northern rim

SWFAS Sept 2016 Newsletter - Southwest Florida Astronomical
SWFAS Sept 2016 Newsletter - Southwest Florida Astronomical

... study the outer Solar System, Voyager 1 launched 16 days after its twin, Voyager 2. Having operated for 38 years, 11 months and 19 days, the spacecraft still communicates with the Deep Space Network to receive routine commands and return data. At a distance of 135 AU (2.02×1010 km) from the Sun as o ...
Martin`s presentation
Martin`s presentation

Chapter 13
Chapter 13

... C) we would still orbit it in a period of one year. D) we would immediately escape into deep space, driven out by its radiation. E) all terrestrial planets would fall in immediately. 34. What is Cygnus X-1? A) a millisecond pulsar with three Earth-like planets around it B) The brightest star in the ...
Observing the Solar Spectrum
Observing the Solar Spectrum

talk - Centre for Astrophysics and Supercomputing
talk - Centre for Astrophysics and Supercomputing

... Galactic Halo Stars in Phase Space: A Hint of Satellite Accretion? Brook, Kawata, Gibson, & Flynn (2003, ApJL in press) ...
ASTRONOMY AND ASTROPHYSICS
ASTRONOMY AND ASTROPHYSICS

... atmosphere, generates an electromagnetic cascade of e+, eÐ and g. These particles, and also the Cerenkov radiation and the fluorescence generated by these relativistic charged particles in the atmosphere can be observed at the ground level. At the highest energies gamma ray astronomy is carried out ...
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X-ray astronomy satellite

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