Search Results - "Nürnberger, Pierre"

How do supernova remnants cool? – I. Morphology, optical emission lines, and shocks by Makarenko, Ekaterina I, Walch, Stefanie, Clarke, Seamus D, Seifried, Daniel, Naab, Thorsten, Nürnberger, Pierre C, Rathjen, Tim-Eric

“…ABSTRACT Supernovae (SNe) inject ∼1051 erg in the interstellar medium, thereby shocking and heating the gas. A substantial fraction of this energy is later…”
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SILCC -- VIII: The impact of far-ultraviolet radiation on star formation and the interstellar medium by Rathjen, Tim-Eric, Walch, Stefanie, Naab, Thorsten, Nürnberger, Pierre, Wünsch, Richard, Seifried, Daniel, Glover, Simon C. O

“…We present magnetohydrodynamic simulations of star formation in the multiphase interstellar medium to quantify the impact of non-ionising far-ultraviolet (FUV)…”
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The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium by Brugaletta, Vittoria, Walch, Stefanie, Naab, Thorsten, Girichidis, Philipp, Rathjen, Tim-Eric, Seifried, Daniel, Nürnberger, Pierre Colin, Wünsch, Richard, Glover, Simon C. O

“…Low-metallicity environments are subject to inefficient cooling. They also have low dust-to-gas ratios and therefore less efficient photoelectric (PE) heating…”
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How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks by Makarenko, Ekaterina I, Walch, Stefanie, Clarke, Seamus D, Seifried, Daniel, Naab, Thorsten, Nürnberger, Pierre C, Rathjen, Tim-Eric

“…Supernovae (SNe) inject $\sim 10^{51}$ erg in the interstellar medium, thereby shocking and heating the gas. A substantial fraction of this energy is later…”
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Synthetic CO emission and the $X_{\rm CO}$ factor of young molecular clouds: a convergence study by Borchert, Elisabeth M. A, Walch, Stefanie, Seifried, Daniel, Clarke, Seamus D, Franeck, Annika, Nürnberger, Pierre

“…The properties of synthetic CO emission from 3D simulations of forming molecular clouds are studied within the SILCC-Zoom project. Since the time scales of…”
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