output
19932026
most citedOn the Absorption of X-rays in the Interstellar Medium

4k citations

Showing 2022 · astro-ph.GAShow all

8 papers · 2 filters

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★ 2 cited

Near-Infrared Spectroscopy of Ultracompact \ion{H}{2} regions in W51A with NIFS/ALTAIR

Cassio L. Barbosa, Felipe Navarete, Robert D. Blum +1

W51A is the most active star formation region of the Giant \ion{H}{2} region W51. It harbors the two massive proto-clusters W51e and W51\,IRS2, which are very rare in the Galaxy. W…

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

Long-term evolution of multimass rotating star clusters

Alexander R. Livernois, Enrico Vesperini, Anna Lisa Varri +2

We investigate the long-term dynamical evolution of the internal kinematics of multimass rotating star clusters. We have performed a set of N-body simulations to follow the interna…

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…