Search Results - "Glover, S C O"

The ISM in spiral galaxies: can cooling in spiral shocks produce molecular clouds? by Dobbs, C. L., Glover, S. C. O., Clark, P. C., Klessen, R. S.

“…We investigate the thermodynamics of the interstellar medium (ISM) and the formation of molecular hydrogen through numerical simulations of spiral galaxies…”
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The SILCC (SImulating the LifeCycle of molecular Clouds) project – I. Chemical evolution of the supernova-driven ISM by Walch, S., Girichidis, P., Naab, T., Gatto, A., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Peters, T., Derigs, D., Baczynski, C.

“…The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-consistently understand the small-scale structure of the interstellar medium…”
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Uncertainties in H2 and HD chemistry and cooling and their role in early structure formation by Glover, S. C. O., Abel, T.

“…At low temperatures, the main coolant in primordial gas is molecular hydrogen, H2. Recent work has shown that primordial gas that is not collapsing…”
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SILCC-Zoom: the dynamic and chemical evolution of molecular clouds by Seifried, D., Walch, S., Girichidis, P., Naab, T., Wünsch, R., Klessen, R. S., Glover, S. C. O., Peters, T., Clark, P.

“…Abstract We present 3D ‘zoom-in’ simulations of the formation of two molecular clouds out of the galactic interstellar medium. We model the clouds – identified…”
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On the relationship between molecular hydrogen and carbon monoxide abundances in molecular clouds by Glover, S. C. O., Low, M.-M. Mac

“…The most usual tracer of molecular gas is line emission from CO. However, the reliability of this tracer has long been questioned in environments different…”
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The density variance-Mach number relation in supersonic turbulence - I. Isothermal, magnetized gas by Molina, F. Z., Glover, S. C. O., Federrath, C., Klessen, R. S.

“…It is widely accepted that supersonic, magnetized turbulence plays a fundamental role for star formation in molecular clouds. It produces the initial dense gas…”
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On the detection of supermassive primordial stars – II. Blue supergiants by Surace, Marco, Zackrisson, Erik, Whalen, Daniel J, Hartwig, Tilman, Glover, S C O, Woods, Tyrone E, Heger, Alexander

“…ABSTRACT Supermassive primordial stars in hot, atomically cooling haloes at z ∼ 15–20 may have given birth to the first quasars in the Universe. Most…”
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Synthetic [C ii] emission maps of a simulated molecular cloud in formation by Franeck, A, Walch, S, Seifried, D, Clarke, S D, Ossenkopf-Okada, V, Glover, S C O, Klessen, R S, Girichidis, P, Naab, T, Wünsch, R, Clark, P C, Pellegrini, E, Peters, T

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Star Formation at Very Low Metallicity. I. Chemistry and Cooling at Low Densities by Glover, S. C. O, Jappsen, A.-K

“…We present a simplified chemical and thermal model designed to allow computationally efficient study of the thermal evolution of metal-poor gas within large…”
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The IMF as a function of supersonic turbulence by Bertelli Motta, C., Clark, P. C., Glover, S. C. O., Klessen, R. S., Pasquali, A.

“…Recent studies seem to suggest that the stellar initial mass function (IMF) in early-type galaxies might be different from a classical Kroupa or Chabrier IMF,…”
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Is H+ 3 cooling ever important in primordial gas? by Glover, S. C. O., Savin, D. W.

“…Studies of the formation of metal-free Population III stars usually focus primarily on the role played by H2 cooling, on account of its large chemical…”
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Star Formation at Very Low Metallicity. II. On the Insignificance of Metal-Line Cooling During the Early Stages of Gravitational Collapse by Jappsen, A.-K, Glover, S. C. O, Klessen, R. S, Mac Low, M.-M

“…We study the influence of low levels of metal enrichment on the cooling and collapse of ionized gas in small protogalactic halos using three-dimensional,…”
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Mapping Metallicity Variations across Nearby Galaxy Disks by Kreckel, K., Ho, I.-T., Blanc, G. A., Groves, B., Santoro, F., Schinnerer, E., Bigiel, F., Chevance, M., Congiu, E., Emsellem, E., Faesi, C., Glover, S. C. O., Grasha, K., Kruijssen, J. M. D., Lang, P., Leroy, A. K., Meidt, S. E., McElroy, R., Pety, J., Rosolowsky, E., Saito, T., Sandstrom, K., Sanchez-Blazquez, P., Schruba, A.

“…The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution…”
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Fervent: chemistry-coupled, ionizing and non-ionizing radiative feedback in hydrodynamical simulations by Baczynski, C., Glover, S. C. O., Klessen, R. S.

“…We introduce a radiative transfer code module for the magnetohydrodynamical adaptive mesh refinement code flash 4. It is coupled to an efficient chemical…”
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The PHANGS–MUSE nebular catalogue by Groves, B, Kreckel, K, Santoro, F, Belfiore, F, Zavodnik, E, Congiu, E, Egorov, O V, Emsellem, E, Grasha, K, Leroy, A, Scheuermann, F, Schinnerer, E, Watkins, E J, Barnes, A T, Bigiel, F, Dale, D A, Glover, S C O, Pessa, I, Sanchez-Blazquez, P, Williams, T G

“…ABSTRACT Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM). Their bright emission lines enable the measurement of…”
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Radiative feedback from ionized gas by Glover, S. C. O.

“…H2 formation in metal-free gas occurs via the intermediate H− or H+ 2 ions. Destruction of these ions by photodissociation therefore serves to suppress H2…”
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WARPFIELD-EMP: The self-consistent prediction of emission lines from evolving H ii regions in dense molecular clouds by Pellegrini, E W, Rahner, D, Reissl, S, Glover, S C O, Klessen, R S, Rousseau-Nepton, L, Herrera-Camus, R

“…ABSTRACT We present the warpfield emission predictor, warpfield-emp, which couples the 1D stellar feedback code warpfield with the cloudy H iiregion/PDR code…”
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Modelling the supernova-driven ISM in different environments by Gatto, A., Walch, S., Low, M.-M. Mac, Naab, T., Girichidis, P., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Baczynski, C., Peters, T., Ostriker, J. P., Ibáñez-Mejía, J. C., Haid, S.

“…We use hydrodynamical simulations in a (256 pc)3 periodic box to model the impact of supernova (SN) explosions on the multiphase interstellar medium (ISM) for…”
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Modelling CO formation in the turbulent interstellar medium by Glover, S. C. O., Federrath, C., Mac Low, M.-M., Klessen, R. S.

“…We present results from high-resolution three-dimensional simulations of turbulent interstellar gas that self-consistently follow its coupled thermal, chemical…”
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On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions by Joshi, P R, Walch, S, Seifried, D, Glover, S C O, Clarke, S D, Weis, M

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