activity
19962026
most citedThe warm ionized medium in spiral galaxies

366 citations · 1.8k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph.GA2026

Interstellar Dust Transport Through the Heliosphere Including the Sector Region

Jonathan D. Slavin, Marc Kornbleuth, Merav Opher +1

Interstellar dust has been detected in situ flowing through the heliosphere. However, our ability to derive the density and size distribution of the interstellar dust in the local…

astro-ph.SR2025

First Resolution of a Main Sequence G-Star Astrosphere Using Chandra

C. M. Lisse, S. J. Wolk, B. Snios +24

We report resolution of a halo of X-ray line emission surrounding the Zero Age Main Sequence (ZAMS) G8.5V star HD 61005 by Chandra ACIS-S. Located only 36.4 pc distant, HD 61005 is…

astro-ph.GA2023★ 5 cited

Infrared Ejecta and Cold Dust in the Young Supernova Remnant N132D

Jeonghee Rho, Aravind P. Ravi, Jonathan D. Slavin +1

We present Spitzer, WISE, and Herschel observations of the young supernova remnant (SNR) N132D in the LMC, including 3-40 microns Spitzer IRS mapping, 12 microns WISE and 70, 100,…

astro-ph.IM2022★ 1 cited

Near-Earth Supernovae in the Past 10 Myr: Implications for the Heliosphere

Jesse A. Miller, Brian D. Fields, Thomas Y. Chen +10

We summarize evidence that multiple supernovae exploded within 100 pc of Earth in the past few Myr. These events had dramatic effects on the heliosphere, compressing it to within ~…

astro-ph.SR2022★ 17 cited

Dust Production in a Thin Dense Shell in Supernovae with Early Circumstellar Interactions

Arkaprabha Sarangi, Jonathan Slavin

In supernovae (SNe), where the light curves show evidence of strong and early interaction between the ejecta and the circumstellar matter (CSM), the formation of new dust is estima…

astro-ph.GA2020★ 21 cited

Turbulence and Particle Acceleration in Radiative Shock Waves in the Cygnus Loop II: Development of Postshock Turbulence

John C. Raymond, Jonathan D. Slavin, William P. Blair +3

Radiative shock waves in the Cygnus Loop and other supernova remnants show different morphologies in [O III] and Hα emission. We use HST spectra and narrowband images to study the…