activity
20102025
most citedProbing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - II. CO line survey of evolved stars: derivation of mass-loss rate formulae

242 citations · 593 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.EP2025

Systematic determination of dust properties for a sample of 133 spatially resolved debris discs

J. P. Marshall, S. Hengst, R. Young +6

Determination of the composition and size distribution of dust grains in debris discs is strongly dependent on constraining the underlying spatial distribution of that dust through…

astro-ph.IM2025

{\sc ampere}: A tool to fit heterogeneous observations consistently

P. Scicluna, S. Zeegers, J. P. Marshall +5

As astronomy advances and data becomes more complex, models and inference also become more expensive and complex. In this paper we present {\sc ampere}, which aims to solve this pr…

astro-ph.GA2025★ 1 cited

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…

astro-ph.SR2025

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

I. McDonald, S. Srinivasan, P. Scicluna +23

We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved…

astro-ph.GA2023★ 27 cited

GOALS-JWST: Pulling Back the Curtain on the AGN and Star Formation in VV 114

J. Rich, S. Aalto, A. S. Evans +33

We present results from the James Webb Space Telescope (JWST) Director's Discretionary Time Early Release Science (ERS) program 1328 targeting the nearby, Luminous Infrared Galaxy…

astro-ph.GA2022★ 69 cited

GOALS-JWST: Mid-Infrared Spectroscopy of the Nucleus of NGC 7469

L. Armus, T. Lai, V. U +32

We present mid-infrared spectroscopic observations of the nucleus of the nearby Seyfert galaxy NGC 7469 taken with the MIRI instrument on the James Webb Space Telescope (JWST) as p…

astro-ph.GA2021

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…

astro-ph.SR2021★ 8 cited

The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds

C. Agliozzo, N. Phillips, A. Mehner +6

(Shortened) Luminous blue variable stars (LBVs) form dust as a result of episodic, violent mass loss. To investigate their contribution as dust producers in the Magellanic Clouds,…

astro-ph.GA2020★ 42 cited

CHIMPS2: Survey description and CO emission in the Galactic Centre

D. J. Eden, T. J. T. Moore, M. J. Currie +103

The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data…

astro-ph.SR2020★ 9 cited

Rapid grain growth in post-AGB disc systems from far-infrared and sub-millimetre photometry

P. Scicluna, F. Kemper, A. Trejo +3

The timescales on which astronomical dust grows remain poorly understood, with important consequences for our understanding of processes like circumstellar disk evolution and plane…

astro-ph.GA2018★ 16 cited

ALMA reveals molecular cloud N55 in the Large Magellanic Cloud as a site of massive star formation

N Naslim, K. Tokuda, T. Onishi +11

We present the molecular cloud properties of N55 in the Large Magellanic Cloud using CO(1-0) and CO(1-0) observations obtained with Atacama Large Millimeter Array. We…

astro-ph.GA2017★ 10 cited

The mineralogy of newly formed dust in active galactic nuclei

Sundar Srinivasan, Franciska Kemper, Yeyan Zhou +8

The tori around active galactic nuclei (AGN) are potential formation sites for large amounts of dust, and they may help resolve the so-called dust budget crisis at high redshift. W…

astro-ph.SR2016

Identifying the chemistry of the dust around AGB stars in nearby galaxies

Sundar Srinivasan, Franciska Kemper, Ronny Zhao-Geisler

Asymptotic giant branch (AGB) stars are significant contributors to the chemical enrichment of the interstellar medium (ISM) of galaxies. It is therefore essential to constrain the…

astro-ph.SR2011★ 169 cited

Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC) II. Cool Evolved Stars

Martha L. Boyer, Sundar Srinivasan, Jacco Th. van Loon +17

We investigate the infrared (IR) properties of cool, evolved stars in the Small Magellanic Cloud (SMC), including the red giant branch (RGB) stars and the dust-producing red superg…

astro-ph.SR2010★ 242 cited

Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - II. CO line survey of evolved stars: derivation of mass-loss rate formulae

E. De Beck, L. Decin, A. de Koter +4

We aim to (1) set up simple and general analytical expressions to estimate mass-loss rates of evolved stars, and (2) from those calculate estimates for the mass-loss rates of asymp…