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Developing post-coronagraphic, high-resolution spectroscopy for terrestrial planet characterization on ELTs
N. Jovanovic, O. Guyon, T. Kotani +12
Spectroscopic observations are extremely important for determining the composition, structure, and surface gravity of exoplanetary atmospheres. High resolution spectroscopy of the…
The K2-HERMES Survey. I. Planet Candidate Properties from K2 Campaigns 1-3
Robert A. Wittenmyer, Sanjib Sharma, Dennis Stello +31
Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host…
bRing: An observatory dedicated to monitoring the Pictoris b Hill sphere transit
R. Stuik, J. I. Bailey, P. Dorval +8
Aims. We describe the design and first light observations from the Pictoris b Ring ("bRing") project. The primary goal is to detect photometric variability from the young star…
Asteroseismic masses of retired planet-hosting A-stars using SONG
D. Stello, D. Huber, F. Grundahl +9
To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of field stars is often difficult.…
Binary Star Formation and the Outflows from their Discs
Rajika Kuruwita, Christoph Federrath, Michael Ireland
We carry out magnetohydrodynamical simulations with FLASH of the formation of a single, a tight binary (2.5 AU) and a wide binary star (45 AU). We study the outflows…
Science cases for a visible interferometer
Philippe Stee, France Allard, Myriam Benisty +54
High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited to a spatial resolutio…