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The Interstellar Environment of our Galaxy [PDF]
Reviews of Modern Physics, 2001 We review the current knowledge and understanding of the interstellar medium
of our galaxy. We first present each of the three basic constituents - ordinary
matter, cosmic rays, and magnetic fields - of the interstellar medium, laying
emphasis on their ...Abbott, D. C., Abbott, D. C., Adams, W. S., Asseo, E., Bakes, E. L. O., Bartunov, O. S., Beals, C. S., Beck, R., Belfort, P., Bell, A. R., Bernard, J.-P., Beuermann, K., Birk, G. T., Blaauw, A., Blandford, R. D., Blandford, R. D., Blitz, L., Blitz, L., Bloemen, H., Bloemen, J. B. G. M., Bloemen, J. B. G. M., Bohlin, R. C., Bohlin, R. C., Bothe, W., Boulanger, F., Boulanger, F., Boulares, A., Branch, D., Bregman, J. N., Breitschwerdt, D., Bronfman, L., Burke, B. F., Burrows, D. N., Burton, W. B., Burton, W. B., Burton, W. B., Cappellaro, E., Carruthers, G., Castor, J., Cesarsky, C. J., Chevalier, R. A., Cioffi, D. F., Clemens, D. P., Cohen, M., Conti, P. S., Cordes, J. M., Cox, D. P., Cox, D. P., Crovisier, J., Crovisier, J., Crutcher, R. M., Cui, W., Dame, T. M., Dame, T. M., Davis, L., Jr., de Jong, T., Dickey, J. M., Dickey, J. M., Dickey, J. M., Diplas, A., Domgörgen, H., Dove, J. B., Dove, J. B., Draine, B. T., Draine, B. T., Duley, W. W., Duley, W. W., Dwek, E., Dwek, E., Dwek, E., Désert, F.-X., Elmegreen, B. G., Elmegreen, B. G., Elmegreen, B. G., Evans, R., Ewen, H. I., Fabbiano, G., Falgarone, E., Falgarone, E., Federman, S. R., Fermi, E., Fermi, E., Ferrière, K. M., Ferrière, K. M., Ferrière, K. M., Ferrière, K. M., Ferrière, K. M., Ferrière, K. M., Fichtel, C. E., Field, G. B., Field, G. B., Franco, J., Freedman, W. L., Freeman, K. C., Frisch, P. C., Frisch, P. C., Fruscione, A., Garcia-Munoz, M., Gardner, F. F., Garmany, C. D., Garwood, R. W., Georgelin, Y. M., Gies, D. R., Ginzburg, V. L., Gleeson, L. J., Goldsmith, D. W., Grabelsky, D. A., Haffner, L. M., Hall, J. S., Han, J. L., Han, J. L., Han, J. L., Harding, D. S., Hartmann, J., Haslam, C. G. T., Haslam, C. G. T., Heiles, C., Heiles, C., Heiles, C., Heiles, C., Heiles, C., Heiles, C., Heiles, C., Heiles, C., Henderson, A. P., Hennebelle, P., Hess, V., Hewish, A., Heyer, M. H., Hillas, A. M., Hiltner, W. A., Hiltner, W. A., Hobbs, L. M., Hollenbach, D. J., Hollenbach, D. J., Howk, J. C., Humphreys, R. M., Hurwitz, M., Inoue, M., Ip, W.-H., Jenkins, E. B., Jenkins, E. B., Jenkins, E. B., Jenkins, E. B., Jenkins, E. B., Johnston, S., Jokipii, J. R., Jokipii, J. R., Jones, A. P., Katz, N., Kennicutt, R. C., Jr., Kerr, F. J., Kim, S.-H., Knacke, R. F., Kulkarni, S. R., Kulsrud, R., Lada, C. J., Lagache, G., Lagache, G., Lagache, G., Larson, R. B., Lin, C. C., Liszt, H. S., Lockman, F. J., Lyne, A. G., Léger, A., Mac Low, M.-M., Magnani, L., Mallik, D. C. V., Maloney, P., Manchester, R. N., Mathewson, D. S., Mathis, J. S., Mathis, J. S., McCammon, D., McClure-Griffiths, N. M, McCray, R., McCray, R., McKee, C. F., McKee, C. F., McKee, C. F., McMillan, R. J., Meyer, D. M., Meyer, J.-P., Miller, G. E., Miller, W. W., Minter, A. H., Moos, H. W., Morton, D. C., Morton, D. C., Mouschovias, T. C., Mouschovias, T. C., Mouschovias, T. C., Mouschovias, T. C., Mueller, M. W., Myers, P. C., Nakano, T., Narayan, R., Narayan, R., Norman, C., Norman, C. A., Oort, J. H., Oren, A. L., Parker, E. N., Parker, E. N., Parravano, A., Piddington, J. H., Potgieter, M. S., Rand, R. J., Rand, R. J., Rasmussen, I. L., Redfield, S., Rees, M. J., Reynolds, R. J., Reynolds, R. J., Reynolds, R. J., Reynolds, R. J., Reynolds, R. J., Reynolds, R. J., Reynolds, R. J., Ristorcelli, I., Rockstroh, J. M., Rogerson, J. B., Salpeter, E. E., Savage, B. D., Savage, B. D., Savage, B. D., Savage, B. D., Savage, B. D., Schaller, G., Schlegel, D. J., Scoville, N. Z., Seab, C. G., Sembach, K. R., Sfeir, D. M., Shapiro, P. R., Shelton, R. L., Shu, F. H., Shull, J. M., Shull, J. M., Shull, J. M., Shull, J. M., Shull, J. M., Silk, J., Simard-Normandin, M., Simpson, J. A., Simpson, J. A., Sivan, J.-P., Sivan, J.-P., Slavin, J. D., Slavin, J. D., Smith, A. M., Snow, T. P., Snowden, S. L., Snowden, S. L., Snowden, S. L., Snowden, S. L., Solomon, P. M., Spitzer, L., Jr., Spitzer, L., Jr., Spitzer, L., Jr., Spitzer, L., Jr., Steenbeck, M., Strong, A. W., Strong, A. W., Struve, O., Tammann, G. A., Taylor, J. H., Tenorio-Tagle, G., Thomson, R. C., Tomisaka, K., Tomisaka, K., Troland, T. H., Trumpler, R. J., Vacca, W. D., Vainshtein, S. I., Valinia, A., Vallée, J.-P., Van Buren, D., van den Bergh, S., van den Bergh, S., Van Steenberg, M. E., Verschuur, G. L., Verschuur, G. L., Vivekanand, M., Wakker, B. P., Wang, Q. D., Wannier, P. G., Watson, W. D., Weaver, R., Webber, W. R., Webber, W. R., Webber, W. R., Weisberg, J. M., Wentzel, D. G., Wentzel, D. G., Williamson, F. O., Wilson, R. W., Witt, A. N., Wolfire, M. G., Woltjer, L., Woolf, N. J., Woosley, S. E., Wright, E. L., York, D. G., York, D. G., Zweibel, E. G. +306 morecore +4 more sourcesInterstellar Turbulence I: Observations and Processes
Annual Review of Astronomy and Astrophysics, 2004 This two-part review summarizes interstellar turbulence and its implications.
The first part begins with diagnostics and energy sources. Turbulence theory is
considered in detail, including the basic fluid equations, solenoidal and
compressible modes ...Elmegreen, Bruce G., Scalo, Johncore +4 more sourcesCosmic-ray driven dynamo in the medium of irregular galaxy [PDF]
, 2009 We investigate the cosmic ray driven dynamo in the interstellar medium of
irregular galaxy. The observations (Chyzy et al. 2000, 2003) show that the
magnetic field in irregular galaxies is present and its value reaches the same
level as in spiral ...Chyży, Chyży, Dominik Bomans, Hanasz, Hubert Siejkowski, Katarzyna Otmianowska-Mazur, Marian Soida, Michał Hanasz +7 morecore +6 more sourcesOn the 3D Curvature and Dynamics of the Musca Filament
The Astrophysical Journal, 2023 Filaments are ubiquitous in the interstellar medium, yet their formation and evolution remain the topic of intense debate. In order to obtain a more comprehensive view of the 3D morphology and evolution of the Musca filament, we model the C ^18 O(2-1 ...Aidan Kaminsky, Lars Bonne, Doris Arzoumanian, Simon Coudé +3 moredoaj +1 more sourceMeasuring interstellar magnetic fields by radio synchrotron emission [PDF]
, 2008 Radio synchrotron emission, its polarization and its Faraday rotation are
powerful tools to study the strength and structure of interstellar magnetic
fields. The total intensity traces the strength and distribution of total
magnetic fields.Battaner, Beck, Beck, Beck, Beck, Beck, Berkhuijsen, Brentjens, Chyży, Chyży, de Avillez, de Jong, Dumke, Elstner, Fletcher, Han, Heiles, Hoernes, Johnston-Hollitt, Klein, Krause, Krause, Lisenfeld, Lisenfeld, Men, Moss, Nieten, Niklas, Patrikeev, Rainer Beck, Soida, Stepanov, Sun, Tabatabaei, Tabatabaei, Tabatabaei, Walsh, Wolleben +37 morecore +1 more sourceCosmic-ray driven dynamo in galaxies [PDF]
, 2011 We present recent developments of global galactic-scale numerical models of
the Cosmic Ray (CR) driven dynamo, which was originally proposed by Parker
(1992).Allen, Berezinskii, D. Wóltanski, H. Kotarba, Hanasz, Hanasz, Hanasz, Hanasz, Hanasz, K. Kowalik, Kowal, M. Hanasz, Schlickeiser, Siejkowski +13 morecore +2 more sourcesTRIANGULATION OF THE INTERSTELLAR MAGNETIC FIELD [PDF]
The Astrophysical Journal, 2015 Determining the direction of the local interstellar magnetic field (LISMF) is important for understanding the heliosphere's global structure, the properties of the interstellar medium, and the propagation of cosmic rays in the local galactic medium. Measurements of interstellar neutral atoms by Ulysses for He and by SOHO/SWAN for H provided some of the N. A. Schwadron, J. D. Richardson, L. F. Burlaga, D. J. McComas, E. Moebius +4 moreopenaire +2 more sourcesTurbulent amplification of interstellar magnetic fields [PDF]
Symposium - International Astronomical Union, 1991 We show that the radiative cooling properties of the interstellar gas lead naturally to a scaling law for the magnetic field of the form B ∝ n1/2, if the magnetic field is amplified by a vigorous injection of turbulent energy due to expanding HII regions, stellar winds, supernova explosions, stellar jets, etc.openaire +1 more source
