The frequency dependence of scattering imprints on pulsar observations by Geyer, M, Karastergiou, A

“…This work provides a framework for interpretation of upcoming low frequency data, both in terms of modelling the interstellar medium and understanding intrinsic emission properties of pulsars.…”

The impact of radio-AGN on star formation across cosmic time by Virdee, J

“…<p>This thesis presents a detailed study of the impact of radio-AGN on star formation and the interstellar medium (ISM) of galaxies across cosmic time. …”

The frequency dependence of scattering imprints on pulsar observations by Geyer, M, Karastergiou, A

“…This work provides a framework for interpretation of upcoming low-frequency data, both in terms of modelling the interstellar medium and understanding intrinsic emission properties of pulsars.…”

Electron acceleration in laboratory-produced turbulent collisionless shocks by Swadling, GF, Grassi, A, Rinderknecht, H, Higginson, DP, Ryutov, DD, Bruulsema, C, Drake, RP, Funk, S, Glenzer, S, Gregori, G, Li, CK, Pollock, BB, Remington, BA, Ross, JS, Rozmus, Sakawa, Y, Spitkovsky, A, Wilks, S, Park

“…Generated by violent interactions of supersonic plasma flows with the interstellar medium, supernova remnant shocks are observed to amplify magnetic fields and accelerate electrons and protons to highly relativistic speeds. …”

Mapping dust in the giant molecular cloud Orion A by Gration, A, Magorrian, S

“…Moreover, it requires minimal assumptions about the statistical properties of the interstellar medium. In fact, we require only a model of the first and second moments of the dust density field. …”

Physical properties and scaling relations of molecular clouds: the effect of stellar feedback by Grisdale, K, Agertz, O, Renaud, F, Romeo, AB

“…We find that efficient stellar feedback is a necessary ingredient in order to develop a realistic interstellar medium, leading to molecular cloud masses, sizes, velocity dispersions, and virial parameters in excellent agreement with MW observations. …”

Fragmentation dynamics of fluorene explored using ultrafast XUV-Vis pump-probe spectroscopy by Garg, D, Lee, JWL, Tikhonov, DS, Chopra, P, Steber, AL, Lemmens, AK, Erk, B, Allum, F, Boll, R, Cheng, X, Düsterer, S, Gruet, S, He, L, Heathcote, D, Johny, M, Kazemi, MM, Köckert, H, Lahl, J, Loru, D, Maclot, S, Mason, R, Müller, E, Mullins, T, Olshin, P, Passow, C, Peschel, J, Ramm, D, Rompotis, D, Trippel, S, Wiese, J, Ziaee, F, Bari, S, Burt, M, Küpper, J, Rijs, AM, Rolles, D, Techert, S, Eng-Johnsson, P, Brouard, M, Vallance, C, Manschwetus, B, Schnell, M

“…Through their infrared emission signature, PAHs have been shown to be ubiquitous in the universe, and they are assumed to play an important role in the chemistry of the interstellar medium. Our experiments track the ionization and dissociative ionization products of fluorene through time-of-flight mass spectrometry and velocity-map imaging. …”

Finite-Correlation-Time Effects in the Kinematic Dynamo Problem by Schekochihin, A, Kulsrud, R

“…Physical applications of this theory include the small-scale kinematic dynamo in the interstellar medium and protogalactic plasmas.…”

Herschel -PACS spectroscopic diagnostics of local ULIRGs: Conditions and kinematics in Markarian 231 by Fischer, J, Sturm, E, González-Alfonso, E, Graciá-Carpio, J, Hailey-Dunsheath, S, Poglitsch, A, Contursi, A, Lutz, D, Genzel, R, Sternberg, A, Verma, A, Tacconi, L

“…The outflow is characterized by extremely high ratios of 18O/16O suggestive of interstellar medium processing by advanced starbursts. © 2010 ESO.…”

The LMC Microlensing Events: Evidence for a Warped and Flaring Milky Way Disk? by Evans, N, Gyuk, G, Turner, MS, Binney, J

“…But, the precursor population must have polluted the interstellar medium with metals, in conflict with current population II abundance. …”

Astrophysical Gyrokinetics: Basic Equations and Linear Theory by Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, Schekochihin, A

“…We briefly outline several of the problems to be addressed by future nonlinear simulations, including particle heating by turbulence in hot accretion flows and in the solar wind, the magnetic and electric field power spectra in the solar wind, and the origin of small-scale density fluctuations in the interstellar medium.…”

Herschel-PACS spectroscopic diagnostics of local ULIRGs: Conditions and kinematics in Markarian 231 by Fischer, J, Sturm, E, Gonzalez-Alfonso, E, Gracia-Carpio, J, Hailey-Dunsheath, S, Poglitsch, A, Contursi, A, Lutz, D, Genzel, R, Sternberg, A, Verma, A, Tacconi, L

“…The outflow is characterized by extremely high ratios of 18O/16O suggestive of interstellar medium processing by advanced starbursts. © 2010 ESO.…”

The distribution and properties of DLAs at z ≤ 2 in the EAGLE simulations by Garratt-Smithson, L, Power, C, Lagos, CDP, Stevens, ARH, Allison, JR, Sadler, EM

“…We find that the covering fraction of DLAs increases at higher redshift; a significant fraction of neutral atomic hydrogen (H I) resides in the outskirts of galaxies with stellar mass ≥1010 M⊙; and the covering fraction of DLAs in the circumgalactic medium (CGM) is enhanced relative to that of the interstellar medium (ISM) with increasing halo mass. Moreover, we find that the mean density of the H I in galaxies increases with increasing stellar mass, while the DLAs in high- and low-halo mass systems have higher column densities than those in galaxies with intermediate halo masses (∼1012 M⊙ at z = 0). …”

The contribution of unresolved sources on the gamma-ray spectrum of molecular clouds by Vecchiotti Vittoria, Peron Giada, Pagliaroli Giulia, Villante Francesco Lorenzo

“…If this signal is associated with the “truly” diffuse emission produced by the interaction of cosmic rays (CRs) with the interstellar medium (ISM) then its observed spectral features can be interpreted as indirect evidence of a CR spectral hardening toward the Galactic center. …”
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Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? by Ana Glidden, Sara Seager, Janusz J. Petkowski, Shuhei Ono

“…Atmospheric carbon isotope ratios will thus have to be compared against the local interstellar medium or, better yet, their host star. A further substantial complication is the limited precision of remote atmospheric measurements using spectroscopy. …”
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Multi-scale dynamics in star-forming regions: The interplay between gravity and turbulence by Traficante Alessio, Fuller Gary A., Duarte-Cabral Ana, Elia Davide, Heyer Mark H., Molinari Sergio, Peretto Nicolas, Schisano Eugenio

“…In this paradigm it is still unclear if it is gravity or turbulence that drives the observed supersonic non-thermal motions during the collapse, in particular in high-mass regions, and at which scales gravity becomes eventually dominant over the turbulence of the interstellar medium. To investigate this problem we have combined the dynamics of a sample of 70 μm-quiet clumps, selected to cover a wide range of masses and surface densities, with the dynamics of the parent filaments in which they are embedded. …”
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The case for an all-sky millimetre survey at subarcminute resolution by Désert François-Xavier, Calvo Martino, Catalano Andrea, Leclercq Samuel, Macias-Perez Juan, Mayet Frédéric, Monfardini Alessandro, Perotto Laurence, Ponthieu Nicolas

“…We describe the main scientific drivers for such a project: the SZ sky, the high-redshift millimetre Universe and the interstellar medium in our Galaxy and the nearby galaxies. …”
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Distribution of dust properties around carbon rich AGB star: IRAS 04427+4951 using  IRIS and  AKARI survey  by Devendra Raj Upadhyay, Trishna Subedi

“…The method and results we present developed can for the study of astrochemistry of interstellar medium. BIBECHANA 18 (2) (2021) 154-163 …”
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Influences on Infrared Spectra of Benzene Ices for Titan, Comets, and Beyond: Annealings, Artifacts, and Isosbestic Points by Reggie L. Hudson, Perry A. Gerakines

“…Infrared (IR) spectra are needed for both laboratory and observational studies of extraterrestrial ices, both within the solar system, such as for trans-Neptunian objects, comets, and Titan, and in the interstellar medium. Here we present new transmission-IR measurements on solid benzene (C _6 H _6 ), the simplest common aromatic compound. …”
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Theory of Fluid Instabilities in Partially Ionized Plasmas: An Overview by Roberto Soler, Roberto Soler, José Luis Ballester, José Luis Ballester

“…Partially ionized plasmas (PIP) are essential constituents of many astrophysical environments, including the solar atmosphere, the interstellar medium, molecular clouds, accretion disks, planet ionospheres, cometary tails, etc., where the ionization degree may vary from very weak ionization to almost full ionization. …”
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