activity
19992025
most citedCrystalline silicate dust around evolved stars II. The crystalline silicate complexes

199 citations · 752 across the 17 of their papers we have counts for

collaborators

17 papers

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.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.IM2021★ 25 cited

METIS: The Mid-infrared ELT Imager and Spectrograph

Bernhard Brandl, Felix Bettonvil, Roy van Boekel +13

The Mid-infrared ELT Imager and Spectrograph (METIS) will provide the Extremely Large Telescope (ELT) with a unique window to the thermal- and mid-infrared (3 - 13 microns). Its si…

astro-ph.IM2014★ 28 cited

The Mid-infrared E-ELT Imager and Spectrograph (METIS)

Bernhard R. Brandl, Markus Feldt, Alistair Glasse +14

METIS will be among the first generation of scientific instruments on the E-ELT. Focusing on highest angular resolution and high spectral resolution, METIS will provide diffraction…

astro-ph.SR2014★ 21 cited

Location and sizes of forsterite grains in protoplanetary disks: interpretation from the Herschel DIGIT programme

K. M. Maaskant, B. L. de Vries, M. Min +4

The spectra of protoplanetary disks contain mid- and far- infrared emission features produced by forsterite dust grains. The spectral features contain information about the forster…

astro-ph.IM2012★ 2 cited

Innovative Technologies for Optical and Infrared Astronomy

C. R. Cunningham, C. J. Evans, F. Molster +3

Advances in astronomy are often enabled by adoption of new technology. In some instances this is where the technology has been invented specifically for astronomy, but more usually…