activity
20242026
most citedVariations in the 6.2 m polycyclic aromatic hydrocarbon band in Active Galactic Nuclei- and Starburst-dominated galaxies

1 citations · 5 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

Low-Frequency Recombination Lines from Galaxies and AGN over Cosmic Time

Kimberly L. Emig, Sergei Balashev, Francoise Combes +10

Radio recombination lines (RRLs) at low frequencies (<10 GHz) can provide a multi-phase view of interstellar gas in nearby galaxies, absorption-line-systems, and AGN. Hydrogen RRLs…

astro-ph.GA2026★ 1 cited

JWST Observations of Starbursts: Dust Processing in the M82 Superwind

Serena A. Cronin, Alberto D. Bolatto, Helena M. Richie +39

We present JWST MIRI and NIRCam imaging of the inner ~5 kpc of the M82 superwind at 0.05-0.375'' (~0.9-6.5 pc) resolution. Targeted filters probe emission from polycyclic aromatic…

astro-ph.GA2026★ 1 cited

Variations in the 6.2 m polycyclic aromatic hydrocarbon band in Active Galactic Nuclei- and Starburst-dominated galaxies

Carla M. Canelo, Dinalva A. Sales, Vitor Avelaneda +3

Polycyclic aromatic hydrocarbons (PAHs) are fundamental to understanding the interstellar medium (ISM) of several astrophysical objects. Normally present in Starburst (SB) galaxies…

astro-ph.GA2025

Observations of Carbon Radio Recombination Lines with the NenuFAR telescope. I. Cassiopeia A and Cygnus A

Lucie Cros, Antoine Gusdorf, Philippe Salomé +26

Carbon Radio Recombination Lines (CRRLs) at decametre wavelengths trace the diffuse phase of the interstellar medium (ISM) of the Galaxy. Their observation allows to measure physic…

astro-ph.GA2025

Expansion Signatures in 35 HII Regions traced by SOFIA [CII] Emission

Timothy Faerber, Loren D. Anderson, Matteo Luisi +6

We analyze the expansion signatures of 35 HII regions mapped in [CII] 158 micron emission by the Stratospheric Observatory for Infrared Astronomy (SOFIA). The [CII] emission primar…

astro-ph.GA2025

Cool dark gas in Cygnus X: The first large-scale mapping of low-frequency carbon recombination lines

Kimberly L. Emig, Pedro Salas, Loren D. Anderson +14

Understanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold HI and…

astro-ph.IM2024★ 1 cited

Star and Planet Formation with the Single Aperture Large Telescope for Universe Studies (SALTUS) Space Observatory

Kamber Schwarz, Alexander Tielens, Joan Najita +10

The Single Aperture Large Telescope for Universe Studies (SALTUS) is a far-infrared space mission concept with unprecedented spatial and spectral resolution. Saltus consists of a 1…

astro-ph.IM2024★ 1 cited

Single Aperture Large Telescope for Universe Studies (SALTUS): Science Overview

Gordon Chin, Carrie M. Anderson, Jennifer Bergner +33

The SALTUS Probe mission will provide a powerful far-infrared (far-IR) pointed space observatory to explore our cosmic origins and the possibility of life elsewhere. The observator…

astro-ph.IM2024★ 1 cited

High-Redshift Extragalactic Science with the Single Aperture Large Telescope for Universe Studies (SALTUS) Space Observatory

Justin Spilker, Rebecca C. Levy, Daniel Marrone +10

This paper presents an overview of the high-redshift extragalactic science case for the Single Aperture Large Telescope for Universe Studies (SALTUS) far-infrared NASA probe-class…

astro-ph.IM2024

Milky Way and Nearby Galaxies Science with the Single Aperture Large Telescope for Universe Studies (SALTUS) Space Observatory

Rebecca C. Levy, Alexander Tielens, Justin Spilker +3

This paper presents an overview of the Milky Way and nearby galaxies science case for the \textit{Single Aperture Large Telescope for Universe Studies} (SALTUS) far-infrared NASA p…