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20242026
most citedAshes of Creation: JWST Uncovers Silicate Dust in Massive Star Clusters

1 citations · 1 across the 2 of their papers we have counts for

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astro-ph.GA2026

Survival of very small carbonaceous dust grains in the inner-CGM of NGC 891 from JWST/MIRI MRS

Jérémy Chastenet, Ilse De Looze, Karl D. Gordon +26

We present new spectroscopic observations of the inner circumgalactic medium (CGM) of NGC 891 taken with the Mid-Infrared Imager/Medium Resolution Spectroscopy instrument onboard J…

astro-ph.GA20251 cited

Ashes of Creation: JWST Uncovers Silicate Dust in Massive Star Clusters

Daniel Maschmann, Bradley C. Whitmore, David A. Thilker +35

Dust production is a fundamental aspect of the baryonic cycle of star formation. It is known that dust is injected into the interstellar medium during early star formation by super…

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.GA2025

The Resolved Structure of a Low Metallicity Photodissociation Region

Ilyse Y. Clark, Karin Sandstrom, Mark Wolfire +14

Photodissociation Regions (PDRs) are key to understanding the feedback processes that shape interstellar matter in galaxies. One important type of PDR is the interface between HII…

astro-ph.GA2024

JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium

Jérémy Chastenet, Ilse De Looze, Monica Relaño +37

We present new JWST observations of the nearby, prototypical edge-on, spiral galaxy NGC 891. The northern half of the disk was observed with NIRCam in its F150W and F277W filters.…

astro-ph.GA2024

Simulated [CII] in high-z galaxies

N. Muñoz-Elgueta, F. Arrigoni Battaia, G. Kauffmann +4

Extended [CII] emission on tens of kpc, also known as a [CII] halo, is being currently reported around z4-6 star-forming galaxies, especially thanks to the statistics of the…