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R Aquarii: Watching a Volatile Stellar Relationship

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In biology, "symbiosis" refers to two organisms that live close to and interact with one another. Astronomers have long studied a class of stars — called symbiotic stars — that co-exist i...

The Anatomy of Orion

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The Orion molecular cloud is a large complex of hot young stars, nebulae, and dark clouds of gas and dust located in the constellation of Orion. Two particularly famous sights in the nig...

New Evidence That All Stars Are Born in Pairs

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Cambridge, MA - Did our Sun have a twin when it was born 4.5 billion years ago?Almost certainly yes -- though not an identical twin. And so did every other Sun-like star in the univers...

Extended Hard X-ray Emission from a Galactic Nucleus

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Supermassive black holes containing millions or even billions of solar-masses of material are found at the nuclei of almost all galaxies. Our Milky Way, for example, has a nucleus with a ...

A Planet Hotter Than Most Stars

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Austin, TX - A newly discovered Jupiter-like world is so hot that it’s stretching the definition of the word "planet."With a day-side temperature of 4,600 Kelvin (more than 7,800 degre...

Understanding Star-Forming Galaxies

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The more stars a typical spiral galaxy contains, the faster it makes new ones. Astronomers call this relatively tight correlation the "galaxy main sequence." The main sequence might be ...

In Memoriam - Patrick Thaddeus

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Colleagues,I am very sorry to report that Pat Thaddeus passed away on April 28 at the age of 84.

Star Forming Filaments

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Interstellar molecular clouds are often seen to be elongated and "filamentary" in shape, and come in a wide range of sizes. In molecular clouds, where stars form, the filamentary structu...
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