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The Hydrogen 21-cm Emission Line
The Hydrogen 21-cm Emission Line

... million years before it undergoes this transition. Even though this is a rare transition, the large amount of hydrogen gas means that enough hydrogen atoms are emitting the 21-cm wavelength radiation at any one given time to be easily detected with radio telescopes. The Milky Way has about 3 billion ...
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... grating A, camera 5 and the long collimator resulting in a resolving power of 38,000 at 6420 Å with the TI-5 CCD, and 32,000 with the F3KB CCD. The CFHT spectra were obtained with the Gecko coudé spectrograph and the Loral 20482 CCD (15 µ pixels) with an effective resolving power of 120,000 at 671 ...
Sky Watcher - Boise Astronomical Society
Sky Watcher - Boise Astronomical Society

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... Way might consist of distant stars. Aristotle (384-322 B.C.), however, believed the Milky Way to be caused by "the ignition of the fiery exhalation of some stars which were large, numerous and close together" and that the "ignition takes place in the upper part of the atmosphere." The Arabian astron ...
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Millisecond Pulsar Binaries at Transition
Millisecond Pulsar Binaries at Transition

... Disk disappearance occurred at the end of 2012 (Bassa et al. 2014) ...
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Corvus (constellation)



Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.
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