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Modeling a Core Collapse Supernova

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Stars greater than eight solar-masses end their lives spectacularly -- as supernovae. These single-star supernovae are called core collapse supernovae because when their dense cores (at t...

Looking for Warm Dark Matter

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In the last century, astronomers studying the motions of galaxies and the character of the cosmic microwave background radiation came to realize that most of the matter in the universe wa...

Imaging a Young, Planet-Forming Disk

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Protoplanetary disks are a natural product of the star formation process. As material in a pre-stellar condensation collapses to form the central star, angular momentum conservation promp...

Modeling Exoplanet Atmospheres

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All atoms and molecules emit distinctive spectral lines across the spectrum, the details of which depend on the internal structures of the species (for example, the vibration and rotation...

Tracer Galaxies Probe the Cosmic Background

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The universe, perhaps surprisingly, is not comprised of galaxies randomly distributed throughout space; that is, it is not very homogeneous. Instead, its galaxies are clustered into disti...

The 2019 Solar Eclipse from 40,000 Feet

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On July 2, scientists from the Center for Astrophysics | Harvard & Smithsonian (CfA) and the National Center for Atmospheric Research (NCAR) successfully flew a high-altitude research...
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