661 citations · 2k across the 17 of their papers we have counts for
18 papers
The structure and characteristic scales of the HI gas in galactic disks
Sami Dib, Jonathan Braine, Maheswar Gopinathan +9
The spatial distribution of the HI gas in galaxies holds important clues on the physical processes that shape the structure and dynamics of the interstellar medium (ISM). In this w…
Thermal and nonthermal dust sputtering in hydrodynamical simulations of the multiphase interstellar medium
Chia-Yu Hu, Svitlana Zhukovska, Rachel S. Somerville +1
We study the destruction of interstellar dust via sputtering in supernova (SN) shocks using three-dimensional hydrodynamical simulations. With a novel numerical framework, we follo…
Iron and silicate dust growth in the Galactic interstellar medium: clues from element depletions
Svitlana Zhukovska, Thomas Henning, Clare Dobbs
The interstellar abundances of refractory elements indicate a substantial depletion from the gas phase, that increases with gas density. Our recent model of dust evolution, based o…
After The Fall: The Dust and Gas in E+A Post-Starburst Galaxies
A. Smercina, J. D. T. Smith, D. A. Dale +11
The traditional picture of post-starburst galaxies as dust- and gas-poor merger remnants, rapidly transitioning to quiescence, has been recently challenged. Unexpected detections o…
The turbulent life of dust grains in the supernova-driven, multi-phase interstellar medium
Thomas Peters, Svitlana Zhukovska, Thorsten Naab +6
Dust grains are an important component of the interstellar medium (ISM) of galaxies. We present the first direct measurement of the residence times of interstellar dust in the diff…
Modelling Dust Evolution in Galaxies with a Multiphase, Inhomogeneous ISM
Svitlana Zhukovska, Clare Dobbs, Edward B. Jenkins +1
We develop a model of dust evolution in a multiphase, inhomogeneous ISM including dust growth and destruction processes. The physical conditions for grain evolution are taken from…
H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
A. Dariush, S. Dib, S. Hony +39
We combine Herschel/SPIRE sub-millimeter (submm) observations with existing multi-wavelength data to investigate the characteristics of low redshift, optically red galaxies detecte…
Can star cluster environment affect dust input from massive AGB stars?
Svitlana Zhukovska, Mykola Petrov, Thomas Henning
We examine the fraction of massive asymptotic giant branch (AGB) stars remaining bound in their parent star clusters and the effect of irradiation of these stars by intracluster ul…
Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. II. Gas-to-Dust Ratio Variations across ISM Phases
Julia Roman-Duval, Karl Gordon, Margaret Meixner +32
The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and lifecycle of dust in galaxies. We examine the relation between dust and gas…
Life Cycle of Dust in the Magellanic Clouds and the Milky Way
Svitlana Zhukovska, Thomas Henning
To a great extent, our understanding of the life cycle of dust is based on the observational and theoretical studies of the Milky Way and the Magellanic Clouds, which will be the t…
Dust origin in late-type dwarf galaxies: ISM growth vs. type II supernovae
Svitlana Zhukovska
We re-evaluate the roles of different dust sources in dust production as a function of metallicity in late-type dwarf galaxies, with the goal of understanding the relation between…
Formation of silicon oxide grains at low temperature
S. A. Krasnokutski, G. Rouille, C. Jager +3
The formation of grains in the interstellar medium, i.e., at low temperature, has been proposed as a possibility to solve the lifetime problem of cosmic dust. This process lacks a…
Gas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range
A. Rémy-Ruyer, S. C. Madden, F. Galliano +17
This paper analyses the behaviour of the gas-to-dust mass ratio (G/D) of local Universe galaxies over a large metallicity range. We combine three samples: the Dwarf Galaxy Survey,…
Dust input from AGB stars in the Large Magellanic Cloud
Svitlana Zhukovska, Thomas Henning
The dust-forming population of AGB stars and their input to the interstellar dust budget of the Large Magellanic Cloud (LMC) are studied with evolutionary dust models with the main…
Protoplanetary Disk Structure With Grain Evolution: the ANDES Model
V. Akimkin, S. Zhukovska, D. Wiebe +5
We present a self-consistent model of a protoplanetary disk: 'ANDES' ('AccretioN disk with Dust Evolution and Sedimentation'). ANDES is based on a flexible and extendable modular s…
Impact of grain evolution on the chemical structure of protoplanetary disks
A. I. Vasyunin, D. S. Wiebe, T. Birnstiel +3
We study the impact of dust evolution in a protoplanetary disk around a T Tauri star on the disk chemical composition. For the first time we utilize a comprehensive model of dust e…
Condensation of MgS in outflows from carbon stars
Svitlana Zhukovska, Hans-Peter Gail
The basic mechanism responsible for the widespread condensation of MgS in the outflows from carbon rich stars on the tip of the AGB is discussed with the aim of developing a conden…
Evolution of interstellar dust and stardust in the solar neighbourhood
Svitlana Zhukovska, Hans-Peter Gail, Mario Trieloff
The abundance evolution of interstellar dust species originating from stellar sources and from condensation in molecular clouds in the local interstellar medium of the Milky Way is…