Initiation of the detonation in the gravitationally confined detonation model of Type Ia supernovae

Inner disc rearrangement revealed by dramatic brightness variations in the young star PV Cep

Inner dusty regions of protoplanetary discs - I. High resolution temperature structure

Inpainting: A powerful interpolation technique for helio- and asteroseismic data

Insights into the Cepheid distance scale

Instabilities in neutron stars with toroidal magnetic fields

Instability of LBV-stars against radial oscillations

Instability of Superfluid Flow in the Neutron Star Core

Instability of Superfluid Flow in the Neutron Star Inner Crust

Instrumental oscillations in RHESSI count rates during solar flares

Integral field spectroscopy of H2 and CO emission in IRAS 18276-1431: evidence for ongoing post-AGB mass loss

Intensity contrast from MHD simulations and from HINODE observations

Interacting Binaries with Eccentric Orbits II. Secular Orbital Evolution Due To Non-Conservative Mass Transfer

Interacting Binaries with Eccentric Orbits. III. Orbital Evolution due to Direct Impact and Self-Accretion

Interacting Binary Star Environments and the W Ser - DPV - Algol Connection

Interaction and Eruption of Two Filaments Observed by Hinode, SOHO, and STEREO

Interaction between Granulation and Small-Scale Magnetic Flux Observed by Hinode

Interactions between Coronal Mass Ejections Viewed in Coordinated Imaging and In Situ Observations

Interactions between magnetohydrodynamic shear instabilities and convective flows in the solar interior

Interactions between reversed granulation, p-modes, and magnetism?