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Do Fast Radio Bursts come from neutron star mergers?

Do Fast Radio Bursts come from neutron star mergers?

by Maria Drout | Jul 29, 2013 | Daily Paper Summaries

Recently, a population of short (a few micro-seconds) and energetic radio bursts were identified at cosmological distances. Today’s paper hypothesizes that these “Fast Radio Bursts” may be created in the final moments of a neutron star merger.

(Not) Detecting Planets around Brown Dwarfs with Radio Waves

(Not) Detecting Planets around Brown Dwarfs with Radio Waves

by Ben Montet | Jul 26, 2013 | Daily Paper Summaries

Forbich, Berger, and Reid attempt to use a large radio array to detect stellar wobbles induced by orbiting planets at larger separations than are usually probed

AR Coating with a Silicon Dicing Saw

AR Coating with a Silicon Dicing Saw

by Kirit Karkare | Jul 23, 2013 | Daily Paper Summaries

Anti-reflection coatings aren’t just for your glasses — telescope lenses need them too! Here we look at a new technique for reducing reflections in lenses made of silicon.

What Can Radio Emission Tell Us About Dark Matter?

What Can Radio Emission Tell Us About Dark Matter?

by Kirit Karkare | Jun 24, 2013 | Daily Paper Summaries

Dark matter particles annihilating could potentially create electrons and positrons, generating continuum synchrotron emission. This paper attempts to find this signature in nearby dwarf galaxies.

Gas and Dust in a Protoplanetary Disk: Turning 2D Data into 3D Models

Gas and Dust in a Protoplanetary Disk: Turning 2D Data into 3D Models

by Erika Nesvold | May 30, 2013 | Daily Paper Summaries

There’s a lot going on in the HD 142527 protoplanetary disk — accretion, gap opening, and a horseshoe-shaped dust ring. The authors of this paper used ALMA to take a closer look at the gas and dust in this busy disk.

Mysterious Gas Clouds between M31 and M33

Mysterious Gas Clouds between M31 and M33

by Jessica Donaldson | May 15, 2013 | Daily Paper Summaries

Seven gas clouds have been found in the region between two galaxies. Are they part of a intergalactic filament or remnants from a past galaxy interaction?

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