The Solar System is embedded in a flow of low-density, warm, and partially ionized
interstellar material that has been sampled directly by in situ measurements of interstellar …

Cosmic dust grains play an important role for the thermal, dynamical, and chemical structure
of the interstellar medium. This is especially true for the star formation process and the late …

Collisions between the winds of solar-like stars and the local interstellar medium result in a
population of hot hydrogen gas surrounding these stars. Absorption from this hot HI can be …

We present an empirical dynamical model of the LISM based on 270 radial velocity
measurements for 157 sight lines toward nearby stars. Physical parameter measurements …

Measurements of stellar mass-loss rates are used to assess how wind strength varies with
coronal activity and age for solar-like stars. Mass loss generally increases with activity, but …

Using an absorption cell, we measured the Doppler shifts of the interstellar hydrogen
resonance glow to show the direction of the neutral hydrogen flow as it enters the inner …

ABSTRACT The Interstellar Boundary Explorer (IBEX) has been directly observing neutral
atoms from the local interstellar medium for the last six years (2009–2014). This paper ties …

Interstellar dust in the heliosphere ADS Classic is now deprecated. It will be completely retired in
October 2019. This page will automatically redirect to the new ADS interface at that point …

We analyze high-resolution spectra of the nearby (1.34 pc) stars alpha Cen A (G2 V) and
alpha Cen B (K1 V), which were obtained with the Goddard High Resolution Spectrograph …

Neutral atom imaging of the interstellar gas flow in the inner heliosphere provides the most
detailed information on physical conditions of the surrounding interstellar medium (ISM) and …