3 papers
astro-ph.GA2025
The Solar System's passage through the Radcliffe wave during the middle Miocene
E. Maconi, J. Alves, C. Swiggum +14
Context. As the Solar System orbits the Milky Way, it encounters various Galactic environments, including dense regions of the interstellar medium (ISM). These encounters can compr…
astro-ph.GA2024
Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
J. D. Soler, S. Molinari, S. C. O. Glover +10
We present a reconstruction of the line-of-sight motions of the local interstellar medium (ISM) based on the combination of a model of the three-dimensional dust density distributi…
astro-ph.GA2024
A 3D Model of the Local Bubble's Magnetic Field: Insights from Dust and Starlight Polarization
Theo J. O'Neill, Alyssa A. Goodman, Juan D. Soler +2
Clustered stellar feedback creates expanding voids in the magnetized interstellar medium known as superbubbles. Although theory suggests that superbubble expansion is influenced by…