35 citations · 56 across the 8 of their papers we have counts for
8 papers
OH/IR stars in the inner Galactic bulge: I. Colour, CO line, and stellar light curve characteristics
H. Olofsson, T. Khouri, S. Muller +11
Stars on the asymptotic giant branch (AGB) play important roles in a number of astronomical contexts. To quantify these roles, it is necessary to establish the mass-loss characteri…
Origin and characterization of super-Earths and sub-Neptunes
Léna Parc, Julia Venturini, François Bouchy +6
Super-Earths and sub-Neptunes represent the most common class of exoplanets discovered to date in our galaxy, yet they have no direct analogues in the Solar System. Since 2014, res…
Long-period transiting exoplanets: advances in detection and characterization
Solène Ulmer-Moll, Babatunde Akinsanmi, Simon Müller
Most detected transiting planets have orbits which would fit within the one of Mercury, exposing them to intense stellar irradiation and interactions that significantly alter their…
Uranus Study Report: KISS
Mark Hofstadter, Ravit Helled, David J. Stevenson +27
Determining the internal structure of Uranus is a key objective for planetary science. Knowledge of Uranus's bulk composition and the distribution of elements is crucial to underst…
Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
Saburo Howard, Ravit Helled, Simon Müller
Revealing the internal composition and structure of giant planets is fundamental for understanding planetary formation. However, the bulk composition can only be inferred through i…
Evolution of Jupiter and Saturn with helium rain
Saburo Howard, Simon Müller, Ravit Helled
Phase separation between hydrogen and helium at high pressures and temperatures leads to the rainout of helium in the deep interiors of Jupiter and Saturn. This process, also known…
Uranus' Complex Internal Structure
Benno A. Neuenschwander, Simon Müller, Ravit Helled
Uranus' bulk composition remains unknown. Although there are clear indications that Uranus' interior is not fully convective, and therefore has a non-adiabatic temperature profile,…
On the hypothesis of an inverted Z-gradient inside Jupiter
Saburo Howard, Tristan Guillot, Steve Markham +6
Models of Jupiter s interior struggle to agree with measurements of the atmospheric composition. Interior models favour a subsolar or solar abundance of heavy elements Z while atmo…