45 citations · 201 across the 10 of their papers we have counts for
10 papers
The Nearby Evolved Stars Survey III: First data release of JCMT CO-line observations
S. H. J. Wallström, P. Scicluna, S. Srinivasan +37
Low- to intermediate-mass (0.88 M) evolved stars contribute significantly to the chemical enrichment of the interstellar medium in the local Universe, making accur…
Properties of shocked dust grains in supernova remnants
F. D. Priestley, H. Chawner, M. J. Barlow +3
Shockwaves driven by supernovae both destroy dust and reprocess the surviving grains, greatly affecting the resulting dust properties of the interstellar medium (ISM). While these…
Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud
Mikako Matsuura, Victoria Ayley, Hannah Chawner +6
With the entire Small Magellanic Cloud (SMC) mapped by the Spitzer Space Telescope and Herschel Space Observatory, we were able to search 8-250 micron images in order to identify i…
The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
P. Scicluna, F. Kemper, I. McDonald +89
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of 850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO (21) and…
Revisiting the dust destruction efficiency of supernovae
F. D. Priestley, H. Chawner, M. Matsuura +3
Dust destruction by supernovae is one of the main processes removing dust from the interstellar medium (ISM). Estimates of the efficiency of this process, both theoretical and obse…
A Galactic Dust Devil: far-infrared observations of the Tornado Supernova Remnant candidate
Hannah Chawner, Alex D. P. Howard, Haley L. Gomez +10
We present complicated dust structures within multiple regions of the candidate supernova remnant (SNR) the `Tornado' (G357.7-0.1) using observations with Spitzer and Herschel. We…
A Complete Catalogue of Dusty Supernova Remnants
Hannah Chawner, Haley Gomez, Mikako Matsuura +9
We search for far-infrared (FIR) counterparts of known supernova remnants (SNRs) in the Galactic plane (360 degrees in longitude and b = +/- 1 deg ) at 70 - 500 micron with Hersche…
Dust masses and grain size distributions of a sample of Galactic pulsar wind nebulae
F. D. Priestley, M. J. Barlow, I. De Looze +1
We calculate dust spectral energy distributions (SEDs) for a range of grain sizes and compositions, using physical properties appropriate for five pulsar wind nebulae (PWNe) from w…
The dust content of the Crab Nebula
I. De Looze, M. J. Barlow, R. Bandiera +7
We have modelled the near-infrared to radio images of the Crab Nebula with a Bayesian SED model to simultaneously fit its synchrotron, interstellar and supernova dust emission. We…
A Catalogue of Galactic Supernova Remnants in the far-infrared: revealing ejecta dust in pulsar wind nebulae
Hannah Chawner, Ken Marsh, Mikako Matsuura +7
We search for far-infrared (FIR) counterparts of known supernova remnants (SNRs) in the Galactic plane (10 deg <| l |< 60 deg) at 70-500 micron using the Herschel Infrared Galactic…