activity
20042026
most citedSpitzer Infrared Spectrographic point source classification in the Small Magellanic Cloud

67 citations · 67 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

Detection of CO ice in the planetary nebula NGC 6302

Charmi Bhatt, Simon W. Cao, Jan Cami +20

Using JWST/MIRI observations, we report the detection of CO ice in the dusty torus of the planetary nebula NGC 6302, an environment generally considered hostile to fragile mole…

astro-ph.GA2025

Detection of CH3+ in the O-rich planetary nebula NGC 6302

Charmi Bhatt, Jan Cami, Els Peeters +33

Planetary nebulae are sites where ejected stellar material evolves into complex molecules, but the precise physical conditions and chemical routes that govern these processes are u…

astro-ph.GA2025

JWST/NIRCam imaging of the Bipolar Planetary Nebula NGC 6537: the (Infra)red Spider, Revealed

Joel Kastner, Paula Moraga Baez, Bruce Balick +5

We present James Webb Space Telescope (JWST) near-infrared (NIRCam) Br, H, [Fe II], and PAH imaging of the molecule-rich, high-excitation bipolar planetary nebula (PN) NGC 6…

astro-ph.IM2025

The PRIMA promise of deciphering interstellar dust evolution with observations of the nearby Universe

Frédéric Galliano, Maarten Baes, Léo Belloir +25

This paper develops a few science cases, using the PRIMA far-IR probe, aimed at achieving several breakthroughs in our understanding of the dust properties and their evolution. We…

astro-ph.SR2025

The JWST/MIRI view of the planetary nebula NGC 6302 I.: a UV irradiated torus and a hot bubble triggering PAH formation

Mikako Matsuura, Kevin Volk, Patrick Kavanagh +34

NGC 6302 is a spectacular bipolar planetary nebula (PN) whose spectrum exhibits fast outflows and highly ionized emission lines, indicating the presence of a very hot central star…

astro-ph.SR201567 cited

Spitzer Infrared Spectrographic point source classification in the Small Magellanic Cloud

Paul M. E. Ruffle, F. Kemper, O. C. Jones +16

The Magellanic clouds are uniquely placed to study the stellar contribution to dust emission. Individual stars can be resolved in these systems even in the mid-infrared, and they a…