O VI in the local interstellar medium by Barstow, M, Boyce, D, Barstow, J, Forbes, A, Welsh, B, Lallement, R

O VI IN THE LOCAL INTERSTELLAR MEDIUM by Barstow, M, Boyce, D, Welsh, B, Lallement, R, Barstow, J, Forbes, A, Preval, S

Pulsar scattering and the ionized interstellar medium by Geyer, M

“…</p> <p>The detected radio wave signals carry with them information of the ionised interstellar medium (IISM) paths they traveled along. The imprints reveal that the pulsar signals we detect travel along multiple paths. …”

Towards simulating star formation in the interstellar medium by Slyz, A, Devriendt, J, Bryan, G, Silk, J

“…As a first step to a more complete understanding of the local physical processes which determine star formation rates (SFRs) in the interstellar medium (ISM), we have performed controlled numerical experiments consisting of hydrodynamical simulations of a kilo-parsec scale, periodic, highly supersonic and "turbulent" three-dimensional flow. …”

Star formation in a multi-phase interstellar medium by Slyz, A, Devriendt, J, Bryan, G, Silk, J

“…This contribution reports on our first efforts to simulate a multiphase interstellar medium on a kiloparsec scale in three dimensions with the stars and gas modeled self-consistently. …”

Evolution of interstellar medium, star formation, and accretion at high redshift by Scoville, N, Lee, N, Bout, P, Diaz-Santos, T, Sanders, D, Darvish, B, Bongiorno, A, Casey, C, Murchikova, L, Koda, J, Capak, P, Vlahakis, C, Ilbert, O, Sheth, K, Morokuma-Matsui, K, Ivison, R, Aussel, H, Laigle, C, McCracken, H, Armus, L, Pope, A, Toft, S, Masters, D

“…ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field. …”

Understanding the large-scale dynamics of the interstellar medium in barred galaxies by Sormani, M

“…<p>We study the large-scale dynamics of the interstellar medium in barred galaxies. The interest in doing this is two-fold. …”

The impact of stellar feedback on the density and velocity structure of the interstellar medium by Grisdale, K, Agertz, O, Romeo, AB, Renaud, F, Read, JI

“…We quantify the density and velocity structure of the interstellar medium using power spectra and compare the simulated galaxies to observed H <span class="small-caps">I</span> in local spiral galaxies from THINGS (The H <span class="small-caps">I</span> Nearby Galaxy Survey). …”

Interstellar medium conditions in z ~ 0.2 Lyman-break analogs by Contursi, A, Baker, A, Berta, S, Magnelli, B, Lutz, D, Fischer, J, Verma, A, Nielbock, M, Grácia Carpio, J, Veilleux, S, Sturm, E, Davies, R, Genzel, R, Hailey-Dunsheath, S, Herrera-Camus, R, Janssen, A, Poglitsch, A, Sternberg, A, Tacconi, L

“…The principal aim of this work is to determine the typical interstellar medium (ISM) properties of z ∼ 1-2 main sequence (MS) galaxies, with stellar masses between 10 9.5 and 10 11 M o , which are currently not easily detectable in all these lines even with ALMA and NOEMA. …”

The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy by Wardlow, J, Cooray, A, Osage, W, Bourne, N, Clements, D, Dannerbauer, H, Dunne, L, Dye, S, Eales, S, Farrah, D, Furlanetto, C, Ibar, E, Ivison, R, Maddox, S, Michałowski, M, Riechers, D, Rigopoulou, D, Scott, D, Smith, M, Wang, L, Werf, P, Valiante, E, Valtchanov, I, Verma, A

“…We target these questions by using Herschel-PACS to examine the conditions in the interstellar medium (ISM) in far-infrared luminous SMGs at z~1-4. …”

Spectropolarimetric constraints on the nature of the 3.4 micron absorber in the interstellar medium by Adamson, A, Whittet, D, Chrysostomou, A, Hough, J, Aitken, D, Wright, G, Roche, P

Spectropolarimetric constraints on the nature of the 3.4 micron absorber in the interstellar medium by Adamson, A, Whittet, D, Chrysostomou, A, Hough, J, Aitken, D, Wright, G, Roche, P

“…Spectropolarimetry of the 3.4 μm aliphatic C-H stretch feature, generally attributed to carbonaceous dust in the diffuse interstellar medium, has been carried out in the line of sight from the Galactic center source Sagittarius A IRS 7. …”

Cold and controlled ion-radical reactions, relevant to the interstellar medium and outer atmosphere by Miossec, C

“…Ion–radical reactions are important for the chemistry happening in the interstellar medium and in certain regions of Earth’s atmosphere, where both temperature and pressure are low. …”

Low-frequency carbon radio recombination lines. II. The diffuse interstellar medium by Salgado, F, Morabito, L, Oonk, J, Salas, P, Toribio, M, Röttgering, H, Tielens, A

“…In the second paper of the series, we have modeled low-frequency carbon radio recombination lines (CRRLs) from the interstellar medium. Anticipating the Low Frequency Array survey of Galactic CRRLs, we focus our study on the physical conditions of the diffuse, cold neutral medium. …”

Properties of Interstellar Medium in Star-Forming Galaxies at z~1.4 revealed with ALMA by Seko, A, Ohta, K, Yabe, K, Hatsukade, B, Akiyama, M, Iwamuro, F, Tamura, N, Dalton, G

“…We conducted observations of 12CO(J = 5-4) and dust thermal continuum emission toward 20 star-forming galaxies on the main sequence at z ∼ 1.4 using ALMA to investigate the properties of the interstellar medium. The sample galaxies are chosen to trace the distributions of star-forming galaxies in diagrams of stellar mass versus star formation rate and stellar mass versus metallicity. …”

Lyman-alpha emission properties of simulated galaxies: interstellar medium structure and inclination effects by Verhamme, A, Dubois, Y, Blaizot, J, Garel, T, Bacon, R, Devriendt, J, Guiderdoni, B, Slyz, A

“…The aim of this paper is to assess the impact of the interstellar medium (ISM) physics on Lyman-alpha (Lya) radiation transfer and to quantify how galaxy orientation with respect to the line of sight alters observational signatures. …”

Interstellar medium. Pseudo-three-dimensional maps of the diffuse interstellar band at 862 nm. by Kos, J, Zwitter, T, Wyse, R, Bienaymé, O, Binney, J, Bland-Hawthorn, J, Freeman, K, Gibson, B, Gilmore, G, Grebel, E, Helmi, A, Kordopatis, G, Munari, U, Navarro, J, Parker, Q, Reid, W, Seabroke, G, Sharma, S, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Williams, M

“…Understanding their origin in the interstellar medium is one of the oldest problems in astronomical spectroscopy, as DIBs have been known since 1922. …”

Faraday tomography of the local interstellar medium with LOFAR: Galactic foregrounds towards IC 342 by Van Eck, C, Haverkorn, M, Alves, M, Beck, R, de Bruyn, A, Enßlin, T, Farnes, J, Ferrière, K, Heald, G, Horellou, C, Horneffer, A, Iacobelli, M, Jelić, V, Martí-Vidal, I, Mulcahy, D, Reich, W, Röttgering, H, Scaife, A, Schnitzeler, D, Sobey, C, Sridhar, S

“…Magnetic fields pervade the interstellar medium (ISM), but are difficult to detect and characterize. …”

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS by Valtchanov, I, Virdee, J, Ivison, R, Swinyard, B, van der Werf, P, Rigopoulou, D, da Cunha, E, Lupu, R, Benford, D, Riechers, D, Smail, I, Jarvis, M, Pearson, C, Gomez, H, Hopwood, R, Altieri, B, Birkinshaw, M, Coia, D, Conversi, L, Cooray, A, De Zotti, G, Dunne, L, Frayer, D, Leeuw, L, Marston, A

...Spinning black holes in a supernova-driven turbulent interstellar medium ... by Dubois, Y, Volonteri, M, Silk, J, Devriendt, J, Slyz, A