output
19942026
most citedThe Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

8k citations

Showing 2018 · astro-ph.EPShow all

14 papers · 2 filters

astro-ph.EP2018★ 20 cited

Deep ALMA Search for CO Gas in the HD 95086 Debris Disc

Mark Booth, Luca Matrà, Kate Y. L. Su +7

One of the defining properties of debris discs compared to protoplanetary discs used to be their lack of gas, yet small amounts of gas have been found around an increasing number o…

astro-ph.EP2018

Disk Winds and the Evolution of Planet-Forming Disks

I. Pascucci, S. Andrews, C. Chandler +1

Disk winds are thought to play an important role in the evolution and dispersal of planet-forming disks. While high-resolution optical and infrared spectroscopy has identified seve…

astro-ph.EP2018

Planetary Bistatic Radar

M. Brozovic, B. J. Butler, Jean-Luc Margot +2

Planetary radar observations offer the potential for probing the properties of characteristics of solid bodies throughout the inner solar system and at least as far as the orbit of…

astro-ph.EP2018★ 4 cited

Potential for Solar System Science with the ngVLA

Imke de Pater, Bryan Butler, R. J. Sault +6

Radio wavelength observations of solar system bodies are a powerful method of probing many characteristics of those bodies. From surface and subsurface, to atmospheres (including d…

astro-ph.EP2018

Science with an ngVLA: Observing the Effects of Chemistry on Exoplanets and Planet Formation

Brett A. McGuire, Edwin Bergin, Geoffrey A. Blake +6

One of the primary mechanisms for inferring the dynamical history of planets in our Solar System and in exoplanetary systems is through observation of elemental ratios (i.e. C/O).…

astro-ph.EP2018★ 86 cited

Submillimetre dust polarisation and opacity in the HD163296 protoplanetary ring system

W. R. F. Dent, C. Pinte, P. C. Cortes +4

We present ALMA images of the sub-mm continuum polarisation and spectral index of the protoplanetary ringed disk HD163296. The polarisation fraction at 870μm is measured to be ~0.9…