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An Over-Massive Black Hole in the Young Universe

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Astronomers generally accept the notion that black holes at the centers of galaxies co-evolve with their host galaxies, and that they have done did so during all cosmic epochs, from the e...

Transition Disks

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A star is typically born with a disk of gas and dust encircling it, from which planets develop as dust grains in the disk collide, stick together and grow. These disks, warmed by the sta...

The Discovery of the Molecule Si-C-Si in Space

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The space between stars is not empty -- it contains a vast reservoir of diffuse material with about 5-10% of the total mass of our Milky Way galaxy. Most of the material is gas, but abou...

Star Formation Near Supermassive Black Holes

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Most if not all galaxies are thought to host a supermassive black hole in their nuclei, a finding that is both one the most important and amazing in modern astronomy. A supermassive black...

The Physical Properties of Dense Molecular Clouds

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Small, dense interstellar clouds of gas and dust, containing hundreds to thousands of solar-masses of material, are suspected of being the precursors to stars and stellar clusters. These...

MINERVA: Hunting for Earth's Twin

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Astronomers are celebrating the dedication of a new planet-hunting telescope known as Minerva. Installed at the Fred Lawrence Whipple Observatory in Arizona, the Minerva project is an arr...

The Ages of Extragalactic Jets

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The longest known highly collimated structures in the universe are the narrow jets that emanate from the vicinity of powerful black holes in certain types of galactic nuclei. These narr...

The Interstellar Medium A Billion Years After the Big Bang

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The first stars and galaxies began forming a few hundred million years after the big bang, and after a billion years their physical processes dominated the evolution of cosmic structure. ...
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