Modelling observable signatures of jet-ISM interaction: thermal emission and gas kinematics [PDF]
Monthly notices of the Royal Astronomical Society, 2022 Relativistic jets are believed to have a substantial impact on the gas dynamics and evolution of the interstellar medium (ISM) of their host galaxies. In this paper, we aim to draw a link between the simulations and the observable signatures of jet-ISM
M. Meenakshi +8 more
semanticscholar +1 more source
The ALMA-ALPAKA survey. I. High-resolution CO and [CI] kinematics of star-forming galaxies at z= 0.5 - 3.5 [PDF]
Astronomy & Astrophysics, 2023 Spatially-resolved studies of the kinematics of galaxies provide crucial insights into their assembly and evolution, enabling to infer the properties of the dark matter halos, derive the impact of feedback on the ISM, characterize the outflow motions. To
F. Rizzo +15 more
semanticscholar +1 more source
GOALS-JWST: Resolving the Circumnuclear Gas Dynamics in NGC 7469 in the Mid-infrared [PDF]
Astrophysical Journal Letters, 2022 The nearby, luminous infrared galaxy NGC 7469 hosts a Seyfert nucleus with a circumnuclear star-forming ring and is thus the ideal local laboratory for investigating the starburst–AGN (active galactic nucleus) connection in detail.
V. U +37 more
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A Galactic Eclipse: The Small Magellanic Cloud Is Forming Stars in Two Superimposed Systems [PDF]
Astrophysical Journal, 2023 The structure and dynamics of the star-forming disk of the Small Magellanic Cloud (SMC) have long confounded us. The SMC is widely used as a prototype for galactic physics at low metallicity, and yet we fundamentally lack an understanding of the ...
C. Murray +24 more
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The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential [PDF]
Monthly notices of the Royal Astronomical Society, 2020 We present a statistical analysis of the gravoturbulent velocity fluctuations in molecular cloud complexes extracted from our ‘Cloud Factory’ Galactic-scale interstellar medium (ISM) simulation suite.
A. Izquierdo +8 more
semanticscholar +1 more source
VALES: VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z ∼ 0.15 [PDF]
Astronomy & Astrophysics, 2020 Context. Spatially resolved observations of the ionized and molecular gas are critical for understanding the physical processes that govern the interstellar medium (ISM) in galaxies. Aims.
J. Molina +11 more
semanticscholar +2 more sources
ALFALFA DISCOVERY OF THE NEARBY GAS-RICH DWARF GALAXY LEO P. V. NEUTRAL GAS DYNAMICS AND KINEMATICS [PDF]
, 2014 We present new H i spectral line imaging of the extremely metal-poor, star-forming dwarf irregular galaxy Leo P. Our H i images probe the global neutral gas properties and the local conditions of the interstellar medium (ISM).
Elijah Z. Bernstein-Cooper +13 more
semanticscholar +1 more source
COMPARING [C ii], H i, AND CO DYNAMICS OF NEARBY GALAXIES [PDF]
, 2016 The H i and CO components of the interstellar medium (ISM) are usually used to derive the dynamical mass of nearby galaxies. Both components become too faint to be used as a tracer in observations of high-redshift galaxies.
W. D. Blok +16 more
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Dynamical modeling and the interactions with the ISM [PDF]
Proceedings of the International Astronomical Union, 2011 This paper is a review of some of the recent modeling efforts to improve our understanding of structure formation and evolution of planetary nebulae including their interaction with the interstellar medium.
W. Steffen
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The effects of stellar dynamics on the X-ray emission of flat early-type galaxies [PDF]
, 2013 Observational and numerical studies gave hints that the hot gaseous haloes of ETGs may be sensitive to the galaxy internal kinematics. By using high resolution 2D hydro simulations, and realistic two-component (stars plus dark matter) axisymmetric galaxy
A. Negri +5 more
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