Milky Way center: Threads of hot gas and magnetic fields | | The bright center of our home galaxy, the Milky Way, is hidden behind dust. But expand our vision (via telescopes and their instruments) to see different kinds of light – different wavelength regimes of the electromagnetic spectrum – and we can see through the dust. Then go a step further and combine several different kinds of “lights.” At that point, astronomers see fascinating new details, leading to new insights. Astronomer Q. Daniel Wang did just this. He used high-energy X-ray data, gathered over 2 decades, combined with new low-energy radio data. The result is an extraordinary new image (above) of our Milky Way's central region. See the image annotated, and watch a movie. | | |
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Why do variable stars brighten and dim? | | When you go out under a starry sky, the stars seem unchanging, eternal, constant. Occasionally you might see a nova or a supernova - apparently "new" stars - but such events usually last only weeks before fading from view, and they are rare (especially supernovae). Apart from those transient reminders that the universe is restless and constantly changing, the stars in the night sky seem to shine with a steady, unwavering light. But many stars are not constant. Their brightness varies over time. Here's what's fascinating about variable stars. | | |
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