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Showing 1 to 20 of 141 for “"Interstellar Medium"”.

  1. Turbulence and structure formation in the interstellar medium

    The interstellar medium (ISM) structure and dynamics are the result of the interplay between many physical processes such as turbulence, gravity, thermal processes, magnetic fields and cosmic rays which determine the modes of molecular cloud and star formation, and which in turn, define the global …

    heid-diss Repository record for Turbulence and structure formation in the interstellar medium (opens in a new tab)

  2. Stochastic histories of dust grains in the interstellar medium

    … of SUperNOva CONdensateS (SUNOCONS) within the Interstellar Medium (ISM). This is done via a Monte Carlo process where refractory dust grains formed within supernova remnants are subjected to the processes of sputtering and collisional fragmentation in the diffuse phase and accretion within the …

    rice Repository record for Stochastic histories of dust grains in the interstellar medium (opens in a new tab)

  3. Interstellar medium properties and star formation in nearby galaxies

    We study the properties of the interstellar medium (ISM) of nearby galaxies from The HI Nearby Galaxy Survey (THINGS) by analyzing the shapes of their HI emission velocity profiles. We apply a stacking method to increase the signal-to-noise (S/N) of the profiles and obtain what we call a super …

    cape-town Repository record for Interstellar medium properties and star formation in nearby galaxies (opens in a new tab)

  4. The interstellar medium and star formation in edge-on galaxies

    … star forming regions and the importance of interstellar gas pressure in controlling the ρH2 /ρHI ratio for two cases: varying and constant velocity dispersions. The Q parameter does not show a clear correlation with massive star formation although Q using varying velocity dispersion shows …

    uiuc Repository record for The interstellar medium and star formation in edge-on galaxies (opens in a new tab)

  5. The Interstellar Medium Along The Life of Sight Toward X Per

    I have used ultraviolet, optical, and radio observations of the B0 V star X Per to analyze the physical conditions within the obscuring diffuse cloud. The ultraviolet data are from the International Ultraviolet Explorer satellite, the optical data are primarily blue echelle spectra, and the radio …

    uiuc Repository record for The Interstellar Medium Along The Life of Sight Toward X Per (opens in a new tab)

  6. Studies of the Ionised Interstellar Medium at Low Radio Frequencies using LOFAR

    … frequencies, their radiation is affected by interstellar propagation effects like dispersion, which causes a frequency-dependent propagation delay that can vary with time when there is relative motion between the Earth, the pulsar and the gas between the two. These effects on the radiation …

    bielefeld Repository record for Studies of the Ionised Interstellar Medium at Low Radio Frequencies using LOFAR (opens in a new tab)

  7. Investigating bursty star formation and interstellar medium conditions in low-mass galaxies

    Low-mass galaxies or dwarf galaxies (galaxies with stellar massM∗<10⁹ᐧ⁵.5M⊙) are the most abundant systems in the universe, and are the progenitors of present-day Milky Way-mass galaxies. Compared to massive galaxies, low-mass galaxies exhibit higher specific star formation rates (sSFR), and have …

    missouri Repository record for Investigating bursty star formation and interstellar medium conditions in low-mass galaxies (opens in a new tab)

  8. Pulse broadening due to multipath scattering of radio waves by the interstellar medium.

    Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1971.

    mit Repository record for Pulse broadening due to multipath scattering of radio waves by the interstellar medium. (opens in a new tab)

  9. On the Chemistry of Molecules Containing Silicon, Phosphorus, and Sulfur in the Interstellar Medium

    The Interstellar Medium (ISM) is an extreme environment that requires a wide range of experimental techniques to investigate its many shades. This thesis presents a collection of studies in Laboratory Astrochemistry aimed at providing new experimental data for astrochemical modeling and probing the …

    trento Repository record for On the Chemistry of Molecules Containing Silicon, Phosphorus, and Sulfur in the Interstellar Medium (opens in a new tab)

  10. Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies

    The distribution and kinematics of HI in the dwarf ellipticals NGC 185 and NGC 205 are significantly different from those in giant ellipticals, so that an internal origin for the gas in the dwarf ellipticals should be considered. Finally, the presence of gas in LGS 3 conflicts with evolutionary …

    uiuc Repository record for Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies (opens in a new tab)

  11. Investigating the cosmic-ray ionization rate in the galactic interstellar medium through observations of H3+

    Observations of H3+ in the Galactic diffuse interstellar medium (ISM) have led to various surprising results, including the conclusion that the cosmic-ray ionization rate (zeta_2) is about 1 order of magnitude larger than previously thought. The present survey expands the sample of diffuse cloud …

    uiuc Repository record for Investigating the cosmic-ray ionization rate in the galactic interstellar medium through observations of H3+ (opens in a new tab)

  12. Growth of unsaturated, cyclic, and polycyclic aromatic hydrocarbons: Reactions under the conditions of the interstellar medium

    … have been long discussed to be carriers of interstellar infrared (IR) emission and ultraviolet (UV) absorption features. Yet, their origin in dense phases of the interstellar medium (ISM), such as molecular clouds, remains unclear. In this work, growth mechanisms based on ion-molecule …

    qucosa-diss

  13. Nuclear Spin Dependence in Reactions of Hydrogen (3+) Ion in the Laboratory and the Interstellar Medium

    … for understanding the deuterium chemistry of the interstellar medium, and for the fundamental chemical physics of these very simple molecules.

    uiuc Repository record for Nuclear Spin Dependence in Reactions of Hydrogen (3+) Ion in the Laboratory and the Interstellar Medium (opens in a new tab)

  14. Exploiting pulsar timing at low radio frequencies: applications to Pulsar Timing Arrays, Interstellar medium and HII regions

    … chromatic propagation effects in the ionised interstellar medium and to refine the modelling of noise processes in Pulsar Timing Array (PTA) analyses. A central element of this thesis is the combination of observations from LOFAR and NenuFAR with higher-frequency data from the European PTA …

    cagliari Repository record for Exploiting pulsar timing at low radio frequencies: applications to Pulsar Timing Arrays, Interstellar medium and HII regions (opens in a new tab)

  15. Studying the Large Scale Structure and interstellar Medium of Galaxies During the Epochs of Peak Cosmic Star formation and Reionization With Infrared Fine Structure Lines

    … (FS) lines from trace metals in the interstellar medium (ISM) of galaxies are valuable diagnostics of the physical conditions in a broad range of astrophysical environments, such gas irradiated by stellar far-ultraviolet (FUV) photons or X-rays from accreting supermassive black holes, …

    penn Repository record for Studying the Large Scale Structure and interstellar Medium of Galaxies During the Epochs of Peak Cosmic Star formation and Reionization With Infrared Fine Structure Lines (opens in a new tab)

  16. Dissociative charge transfer of organic molecules induced by collisions with the He+ cation. A joint experimental and theoretical study of relevance for the interstellar medium evolution

    … destruction of complex organic molecules in the interstellar medium (ISM). We have carried out dissociative charge transfer reactions of He+ with two oxygen containing organic molecules, ubiquitous in ISM: dimethyl ether (DME, CH3OCH3 ) and methyl formate (MF, HCOOCH3). Since they have a …

    trento Repository record for Dissociative charge transfer of organic molecules induced by collisions with the He+ cation. A joint experimental and theoretical study of relevance for the interstellar medium evolution (opens in a new tab)

  17. Quantum Mechanical Study of Spin-Forbidden Reactions in Organometallic Catalysis and Astrochemistry

    … in organometallic C-H bond activation and interstellar peptide-bond formation, as well as the derivation of the Morse empirical potential from an electrostatic model. In the first part, the role of triplet electronic state in spin-accelerated iron-catalyzed C(sp2)-H bond activation in …

    unr Repository record for Quantum Mechanical Study of Spin-Forbidden Reactions in Organometallic Catalysis and Astrochemistry (opens in a new tab)

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