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Interstellar Lithium in the Small Magellanic Cloud

Interstellar Lithium in the Small Magellanic Cloud

by Kirit Karkare | Jul 17, 2012 | Daily Paper Summaries

What can a nearby dwarf galaxy tell us about the the chemical evolution of the universe?

A new tool to investigate a century old mystery

A new tool to investigate a century old mystery

by Nathan Sanders | Jul 9, 2012 | Daily Paper Summaries

The current and next generation of large scale spectroscopic surveys could provide new clues in the hunt for the carriers producing mysterious interstellar absorption features.

Lessons from Lithium

Lessons from Lithium

by Courtney Dressing | Jul 5, 2012 | Daily Paper Summaries

Is there a link between lithium abundance, galactic chemical evolution, and exoplanets? Ramirez et al. examine metallicities, lithium abundances, and stellar characteristics of 1381 Sun-like stars to find out.

How Common Are Long-Period Jupiters Around Massive Stars?

How Common Are Long-Period Jupiters Around Massive Stars?

by Courtney Dressing | Jun 22, 2012 | Daily Paper Summaries

What fraction of massive stars host gas giants? Vigan et al. observe a sample of A and F stars to find out.

How to count stars you can’t see: the stellar IMF in distant galaxies

How to count stars you can’t see: the stellar IMF in distant galaxies

by Kim Phifer | Jun 8, 2012 | Daily Paper Summaries

Van Dokkum & Conroy examane the variation of the stellar initial mass function by observing the integrated light from early-type galaxies.

This star lives in exciting times, or, How did Betelgeuse make that funny shape?

This star lives in exciting times, or, How did Betelgeuse make that funny shape?

by Elisabeth Newton | Apr 26, 2012 | Daily Paper Summaries

Sometimes we see strange shapes when we look through our fancy telescopes and we’re left wondering how they formed. How did the rings and “pearls” of SN1987A form? Or the hexagonal cloud pattern on Saturn? The star Betelgeuse – famous for being Orion’s left shoulder – presents another unusual geometric appearance.

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