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Self-Generated Magnetic Fields in Galactic Cooling Flows [PDF]
, 1997 Interstellar magnetic fields in elliptical galaxies are assumed to have their
origin in stellar fields that accompany normal mass loss from an evolving
population of old stars.Burn B. J., Cappelaro E., Fabrizio Brighenti, Garrington S. T., Garrington S. T., Jafelice L. C., Lesch H., Lesch H., Moss D., Rees M., Strom R. G., Thomas P. A., William G. Mathews +12 morecore +2 more sourcesCosmic-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 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 sourceThe Interstellar Environment of our Galaxy [PDF]
, 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 +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 sourceBiermann Mechanism in Primordial Supernova Remnant and Seed Fields
, 2006 We have studied the generation of magnetic fields by the Biermann mechanism
in the pair-instability supernovae explosions of the first stars. The Biermann
mechanism produces magnetic fields in the shocked region between the bubble and
interstellar medium Abel, Amjad, Ando, Athreya, Balsara, Biermann, Bromm, Davies, Ferrière, Fosalba, Freyer, Fryer, Gnedin, Han, Hanayama, Hanayama, Kulsrud, Miranda, Mori, Omukai, Pelló, Plaga, Poezd, Raymond, Ricotti, Schneider, Takahashi, Tsagas, Widrow, Yamazaki +29 morecore +1 more source
