Results 11 to 20 of about 104,753 (270)
The turbulent interstellar medium [PDF]
Comptes Rendus. Physique, 2006 An overview is presented of the main properties of the interstellar medium. Evidence is summarized that the interstellar medium is highly turbulent, driven on different length scales by various energetic processes. Large-scale turbulence determines the formation of structures like filaments and shells in the diffuse interstellar medium.Andreas Burkert, Balbus, Ballesteros-Paredes, Bergin, Blitz, Blondin, Bonnell, Burkert, Burkert, Burkert, Cappellaro, Cowie, de Avillez, de Avillez, Dib, Dib, Dickey, Dickey, Dziourkevitch, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Falgarone, Field, Field, Forster Schreiber, Gazol, Hartmann, Hartmann, Hartmann, Hartmann, Heiles, Heitsch, Heitsch, Hennebelle, Hennebelle, Jenkins, Kanekar, Kerp, Kessel-Deynet, Kim, Kim, Kim, Klein, Klessen, Kolmogorov, Koyama, Kritsuk, Kritsuk, Larson, Mac Low, Mac Low, Mac Low, McKee, Palla, Piontek, Puche, Rhode, Scalo, Scalo, Sellwood, Slyz, Stone, Tran, Vishniac, von Weizsäcker, Vázquez-Semadeni, Wada, Walder, Walder, Williams +73 moreopenaire +7 more sourcesOn Graphene in the Interstellar Medium [PDF]
The Astrophysical Journal, 2017 Abstract The possible detection of C24, a planar graphene that was recently reported to be in several planetary nebulae by García-Hernández et al., inspires us to explore whether and how much graphene could exist in the interstellar medium (ISM) and how it would reveal its presence through its ultraviolet (UV) extinction and infrared (IR)X. H. Chen, X. H. Chen, Ke Zhang, Aigen Li +3 moreopenaire +4 more sourcesThe 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 sourcesA future interstellar probe on the dynamic heliosphere and its interaction with the very local interstellar medium: In-situ particle and fields measurements and remotely sensed ENAs
Frontiers in Astronomy and Space Sciences, 2023 The recently published Interstellar Probe (ISP) study report describes a pragmatic mission concept with a launch window that starts in 2036 and is expected to reach several hundreds of astronomical units past the heliopause within a time frame of ≥50 ...K. Dialynas, V. J. Sterken, P. C. Brandt, L. Burlaga, D. B. Berdichevsky, D. B. Berdichevsky, R. B. Decker, S. Della Torre, R. DeMajistre, A. Galli, M. Gkioulidou, M. E. Hill, S. M. Krimigis, S. M. Krimigis, M. Kornbleuth, W. Kurth, B. Lavraud, R. McNutt, D. G. Mitchell, P. S. Mostafavi, R. Nikoukar, M. Opher, E. Provornikova, E. C. Roelof, P. G. Rancoita, J. D. Richardson, E. Roussos, J. M. Sokół, G. La Vacca, J. Westlake, T. Y. Chen +30 moredoaj +1 more sourceInfrared Emission from Interstellar Dust. II. The Diffuse Interstellar
Medium [PDF]
, 2001 We present a quantitative model for the infrared emission from dust in the
diffuse interstellar medium. The model consists of a mixture of amorphous
silicate grains and carbonaceous grains, each with a wide size distribution
ranging from molecules ...Aigen Li, Allain T., Allamandola L. J., B. T. Draine, Boulanger F., Boulanger F., Boulanger F., Cesarsky D., Cesarsky D., Desert F. X., Desert F. X., Duley W. W., Duley W. W., Habing H. J., Hong S. S., Jones A. P., Jones A. P., Kurtz J., Leger A., Leger A., Li A., Mathis J. S., Mattila K., Mattila K., Morgan D. H., Moutou C., Moutou C., Omont A., Onaka T., Pauzat F., Reach W. T., Roche P. F., Roche P. F., Roelfsema P. R., Schutte W. A., Siebenmorgen R., Sturm E., Tanaka M., van der Zwet G. P., Webster A. +39 morecore +3 more sourcesPhosphorus in the diffuse interstellar medium [PDF]
Astronomy & Astrophysics, 2005 We present FUSE and HST/STIS measurements of the PII column density toward Galactic stars. We analyzed PII through the profile fitting of the unsaturated $ $1125 and $ $1533 lines and derived column densities integrated along the sightlines as well as in individual resolved components.Lebouteiller, Vianney, André, Martial, Ferlet, R. +2 moreopenaire +4 more sourcesMapping The Interstellar Medium With Near-Infrared Diffuse Interstellar Bands [PDF]
, 2015 We map the distribution and properties of the Milky Way's interstellar medium as traced by diffuse interstellar bands (DIBs) detected in near-infrared stellar spectra from the SDSS-III/APOGEE survey.Bizyaev, Dmitry, Garcia-Hernandez, D. Anibal, Hayden, M. R., Holtzman, Jon, Johnson, John A., Kinemuchi, K., Majewski, Steven R., Menard, B., Nidever, David L., Perez, A. E. G., Shetrone, Matthew, Wilson, J. C., Zasowski, Gail +12 morecore +1 more source
