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An Accreting Black Hole

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Black holes are often the sources of powerful emission despite their reputation for being implacable sinks for matter and energy. A black hole can be ringed by a disk of matter, and when...

Seyfert Galaxies

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Seyfert galaxies are quite similar to normal galaxies like our own Milky Way except in one critical respect: their nuclei are fantastically bright -- in some instances as luminous as 100...

The Geometry of Coronal Flares Around Another Star

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The corona of a star is the hot, gaseous outer region of its atmosphere. The sun's corona is over a million kelvin, and in some stars can be even ten times hotter. In sun-like stars the c...

Donut Holes in the Young Solar System

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In its infancy, before its planets formed, our sun was ringed by a disk of gas and dust. Astronomers estimate that the dust in this preplanetary disk coagulated and began forming structu...

Twisting in the Wind

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The process of star formation, once thought to involve just the simple coalescence of material under the influence of gravity, is now known to incorporate an exceedingly complex series of...

The Mysterious Born-Again Nebula

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About seven and one-half billion years from now, our sun will have converted nearly all of its hydrogen fuel into helium through fusion, and then burned most of that helium into carbon an...

More Than Half of Sun-like Stars May Have Rocky Planets

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Cambridge, MA Astronomers have discovered that rocky, terrestrial planets might orbit many, if not most, of the nearby sun-like stars in the disk of our galaxy. These new results suggest...

The Birth of a Stellar Cluster

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On average, one new star a year is born in a nursery somewhere in our Milky Way galaxy, at least according to the best current approximations. Stellar nurseries are located in giant clou...
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