activity
20012026
most citedSilicate features in Galactic and extragalactic post-AGB discs

95 citations · 504 across the 10 of their papers we have counts for

collaborators

10 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.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.SR2013★ 90 cited

Physical Properties of Fullerene-containing Galactic Planetary Nebulae

Masaaki Otsuka, F. Kemper, J. Cami +2

We searched the Spitzer Space Telescope data archive for Galactic planetary nebulae (PNe), that show the characteristic 17.4 and um features due to C60, also known as buckminsterfu…

astro-ph.SR2011★ 95 cited

Silicate features in Galactic and extragalactic post-AGB discs

C. Gielen, J. Bouwman, H. Van Winckel +7

Aims. In this paper we study the Spitzer and TIMMI2 infrared spectra of post-AGB disc sources, both in the Galaxy and the LMC. Using the observed infrared spectra we determine the…

astro-ph.CO2011★ 21 cited

The Spitzer discovery of a galaxy with infrared emission solely due to AGN activity

S. Hony, F. Kemper, Paul M. Woods +14

We present a galaxy (SAGE1CJ053634.78-722658.5) at a redshift of 0.14 of which the IR is entirely dominated by emission associated with the AGN. We present the 5-37 um Spitzer/IRS…

astro-ph.GA2010★ 70 cited

The 9.7 and 18 um silicate absorption profiles towards diffuse and molecular cloud lines-of-sight

J. M. van Breemen, M. Min, J. E. Chiar +8

Studying the composition of dust in the interstellar medium (ISM) is crucial in understanding the cycle of dust in our galaxy. The mid-infrared spectral signature of amorphous sili…