activity
19952026
most citedNew Mass Loss Measurements from Astrospheric Lyman-alpha Absorption

469 citations · 8k across the 108 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2026

Why is there cold gas inside the Local Bubble?

Tim-Eric Rathjen, Jeffrey L. Linsky

The Local Bubble (LB) extends approximately 100--200~pc from the Sun and contains ~K plasma and warm photoionised gas. Yet the Local Leo Cold Cloud (LLCC) and the Local Ribbo…

astro-ph.GA2025★ 7 cited

The Origin of the Cluster of Local Interstellar Clouds

Catherine Zucker, Seth Redfield, Sara Starecheski +2

The interstellar medium within of the Sun consists of a complex of fifteen diffuse, partially ionized clouds. Located within the Local Bubble, these clouds, k…

astro-ph.GA2022★ 6 cited

Are the heliosphere, very local interstellar medium, and local cavity in pressure balance with Galactic gravity

Jeffrey L. Linsky, Eberhard Moebius

The Voyager spacecraft are providing the first in situ measurements of physical properties in the outer heliosphere beyond the heliopause. These data, together with data from the I…

astro-ph.GA2022★ 33 cited

Mixing Interstellar Clouds Surrounding the Sun

Paweł Swaczyna, Nathan A. Schwadron, Eberhard Möbius +9

On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in…

astro-ph.GA2022★ 22 cited

Inhomogeneity within Local Interstellar Clouds

Jeffrey L. Linsky, Seth Redfield, Diana Ryder +1

Analysis of interstellar absorption lines observed in high-resolution {\em HST} spectra of nearby stars provides temperatures, turbulent velocities, and kinetic properties of warm…

astro-ph.GA2022★ 1 cited

Inhomogeneity in the Local ISM and its Relation to the Heliosphere

Jeffrey Linsky, Seth Redfield, Diana Ryder +1

This paper reviews past research and new studies underway of the local interstellar environment and its changing influence on the heliosphere. The size, shape, and physical propert…