Orbital eccentricity (in e2) versus semi-major axis for the planet sample with eccentricities constrained to better than 40% for clarity (or if e 0.1). Colors denote sub-Neptunes (1–4 R⊕, blue),
Orbital eccentricity (in e2) versus semi-major axis for the planet sample with eccentricities constrained to better than 40% for clarity (or if e 0.1). Colors denote sub-Neptunes (1–4 R⊕, blue),
AtubAB dynamic instability revealed by TIRF microscopy. (A) Inset: assay design; biotinylated, GMPCPP-stabilised AtubAB dimers (labelled with 20% Alexa Fluor 647, shown as red) were anchored via NeutrAvidin to PEG
Simulation results of abundance ratios / (black lines), / (orange lines), and / (blue lines) with our model (model A) at 16 K (solid lines) and 77 K (dashed lines).






