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Highly excited and concentrated: an academic stereotype or the gas in a galaxy?

Highly excited and concentrated: an academic stereotype or the gas in a galaxy?

by Olivia Cooper | Oct 18, 2022 | Daily Paper Summaries

Much like some astronomers, this distant galaxy keeps the lights on by maintaining high excitement and a central concentration (of hot gas)

Quench your inner star formation

Quench your inner star formation

by Olivia Cooper | Sep 10, 2022 | Daily Paper Summaries

Does one galaxy’s star formation quench another’s? Find out in today’s astrobite.

Bright galaxies blowing bubbles

Bright galaxies blowing bubbles

by Olivia Cooper | Aug 6, 2022 | Daily Paper Summaries

Today’s paper takes a clear view of bubbles blown by bright galaxies in the Epoch of Reionization

Big, bright, bursty, AND early: what are the odds?

Big, bright, bursty, AND early: what are the odds?

by Olivia Cooper | Jun 7, 2022 | Daily Paper Summaries

Just how rare is this hyperluminous heavily obscured active galactic nucleus in a dusty starburst in the early Universe?

Explaining Ancient Stellar Populations

Explaining Ancient Stellar Populations

by Caitlin Doughty | Aug 30, 2019 | Daily Paper Summaries

Why do some dwarf galaxies exhibit such old stellar populations? Perhaps simulations of reionization including radiative transfer can help to explain this peculiar trait.

The First Molecule in the Universe

The First Molecule in the Universe

by Charles Law | Jul 30, 2019 | Daily Paper Summaries

SOFIA observations have detected HeH+ in the planetary nebula NGC 7027, shedding new light on the dawn of chemistry in the universe.

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