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PublicationWe measure and analyze the inflows and outflows of mass, energy, and metals through the interstellar medium (ISM) and circumgalactic medium (CGM) of galaxies in the IllustrisTNG100 simulations …
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PublicationObservations in the Galaxy and nearby spirals have established that the H I-to-H\(_{2}\) transition at solar metallicity occurs at gas weight of P …
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PublicationSimulations predict that circumgalactic hydrogen gas surrounding massive (\(M_{\rm{halo}}^{z=1}=10^{12}-10^{13}\ M_{\odot}\)) galaxies at \(z\sim4\) may be predominantly neutral, and …
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PublicationWe present a very deep CO(3─2) observation of a massive, gas-rich, main sequence, barred spiral galaxy at z ≍ 1.52. Our data were taken with the …
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PublicationCosmic noon represents the prime epoch of galaxy assembly, and a sweet spot for observations with the James Webb Telescope (JWST) and ground-based near-IR integral-field …
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PublicationWe present a detailed kinematic study of a sample of 32 massive (9.5 ⩽ log(M\(_{*}\)/M\(_{\odot}\)) ⩽ 10.9) main sequence star-forming galaxies (MS SFGs) at …
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PublicationThe escape of LyC photons emitted by massive stars from the dense interstellar medium (ISM) of galaxies is a key bottleneck for cosmological reionization. The escape fraction varies …
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PublicationGalaxies at redshift z ∼ 1–2 display high star formation rates with elevated cold gas fractions and column densities. Simulating a self-regulated interstellar medium (ISM) in a …
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PublicationMolecular clouds (MCs) are the birthplaces of new stars in galaxies. A key component of MCs are photodissociation regions (PDRs), where far-ultraviolet radiation plays a crucial role …
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PublicationWe present an analysis of millimeter CO observations to search and quantify signatures of molecular gas outflows. We exploit the large sample of …
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PublicationSpatially-resolved emission line kinematics are invaluable to investigating fundamental galaxy properties and have become increasingly accessible for galaxies at \(z\gtrsim0.5\) through sensitive near-infrared imaging …
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PublicationMolecular hydrogen (H\(_2\)) formation and dissociation are key processes that drive the gas lifecycle in galaxies. Using the SImulating the LifeCycle of Molecular Clouds (SILCC) zoom-in …
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PublicationWe analyze measurements of the thermal Sunyaev-Zeldovich (tSZ) effect arising in the circumgalactic medium (CGM) of \(L^*\) galaxies, reported by Bregman et al. 2022 and Das et …
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PublicationWe present a set of controlled hydrodynamical simulations to study the effects of strong galactic outflows on the density and temperature structures, and associated X-ray signatures, of …
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PublicationThe [CII] 157.74 \(\mu\)m fine structure transition is one of the brightest and most well-studied emission lines in the far-infrared (FIR), produced in the …
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PublicationWe extend the analytic theory presented by Sternberg et al. and Bialy & Sternberg for the production of atomic hydrogen (H I) via far-ultraviolet (FUV) photodissociation at the …
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PublicationThe angular size of the broad line region (BLR) of the nearby active galactic nucleus (AGN) NGC 3783 has been spatially resolved by recent observations with VLTI/GRAVITY …
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PublicationWe introduce a new general-purpose time-dependent ionisation network (IN) and a radiation transport (RT) module in the magneto-hydrodynamic (MHD) code PLUTO. Our ionisation network is …
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PublicationWe present near-infrared interferometric data on the Seyfert 2 galaxy NGC 1068, obtained with the GRAVITY instrument on the European Southern Observatory Very Large Telescope Interferometer. The …
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PublicationSupersonic turbulence results in strong density fluctuations in the interstellar medium (ISM), which have a profound effect on the chemical structure. Particularly useful probes of the diffuse ISM …
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PublicationWe present a 0.16% precise and 0.27% accurate determination of R0, the distance to the Galactic Center. Our measurement uses the star S2 on its 16 …