Physics of the interstellar medium/ by 209514 Dyson, J. E.

Physical processes in the interstellar medium/ by 207904 Spitzer, Lyman

Molecular collisions in the interstellar medium / by Flower, D. R. (David Roger), 1945-

MOLECULAR COLLISIONS IN THE INTERSTELLAR MEDIUM / by Flower, D. R. (David Roger), 1945-, author

The physics and chemistry of the interstellar medium / by 187995 Tien, Cheh Onn

Thermal instability in the interstellar medium by J. Ghanbari, M. Shadmehri

Subjects: “…Interstellar medium…”
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The Interstellar Medium of Dwarf Galaxies by Christian Henkel, Leslie K. Hunt, Yuri I. Izotov

“…This review focuses on the physical and chemical properties of the interstellar medium of those dwarfs that are known to host significant amounts of gas and dust. …”
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Plasmoid Instability in the Multiphase Interstellar Medium by Drummond B. Fielding, Bart Ripperda, Alexander A. Philippov

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Shocks in the Very Local Interstellar Medium by Mostafavi, P., Burlaga, L. F., Cairns, I. H., Fuselier, S. A., Fraternale, F., Gurnett, D. A., Kim, T. K., Kurth, W. S., Pogorelov, N. V., Provornikova, E., Richardson, J. D., Turner, D. L., Zank, G. P.

“…Abstract Large-scale disturbances generated by the Sun’s dynamics first propagate through the heliosphere, influence the heliosphere’s outer boundaries, and then traverse and modify the very local interstellar medium (VLISM). The existence of shocks in the VLISM was initially suggested by Voyager observations of the 2-3 kHz radio emissions in the heliosphere. …”
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The Heliosphere in the Local Interstellar Medium: Into the Unknown by Richardson, John D., Bykov, Andrei, Effenberger, Frederic, Scherer, Klaus, von Steiger, Rudolf, Sterken, Veerle J., Zank, Gary P.

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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. …”

The Fate of the Interstellar Medium in Early-type Galaxies. III. The Mechanism of Interstellar Medium Removal and the Quenching of Star Formation by Michał J. Michałowski, C. Gall, J. Hjorth, D. T. Frayer, A.-L. Tsai, K. Rowlands, T. T. Takeuchi, A. Leśniewska, D. Behrendt, N. Bourne, D. H. Hughes, M. P. Koprowski, J. Nadolny, O. Ryzhov, M. Solar, E. Spring, J. Zavala, P. Bartczak

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Radio wave scattering in the interstellar medium : proceedings/ by Cordes, M. James, Rickett, Barney J., Backer, Donald D., American Institute of Physics, Workshop on Radio Wave Scattering in the Interstellar Medium (1988 : San Diego, California, United States)

The Distribution of Metallicities in the Local Galactic Interstellar Medium by Adam M. Ritchey, Edward B. Jenkins, J. Michael Shull, Blair D. Savage, S. R. Federman, David L. Lambert

Subjects: “…Interstellar medium…”
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Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium by Richardson, J. D., Burlaga, L. F., Elliott, H., Kurth, W. S., Liu, Y. D., von Steiger, R.

“…Abstract The Voyager spacecraft have left the heliosphere and entered the interstellar medium, making the first observations of the termination shock, heliosheath, and heliopause. …”
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Voyager observations of the interaction of the heliosphere with the interstellar medium by Richardson, John D.

“…This paper provides a brief review and update on the Voyager observations of the interaction of the heliosphere with the interstellar medium. Voyager has found many surprises: (1) a new energetic particle component which is accelerated at the termination shock (TS) and leaks into the outer heliosphere forming a foreshock region; (2) a termination shock which is modulated by energetic particles and which transfers most of the solar wind flow energy to the pickup ions (not the thermal ions); (3) the heliosphere is asymmetric; (4) the TS does not accelerate anomalous cosmic rays at the Voyager locations; and (5) the plasma flow in the Voyagers 1 (V1) and 2 (V2) directions are very different. …”
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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. …”

Photocleavage of Aliphatic C–C Bonds in the Interstellar Medium by Guillermo Tajuelo-Castilla, Jesús I. Mendieta-Moreno, Mario Accolla, Jesús M. Sobrado, Sofia Canola, Pavel Jelínek, Gary J. Ellis, José Ángel Martín-Gago, Gonzalo Santoro

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