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Showing 1 to 20 of 68 for “"Neutral Hydrogen"”.

  1. Neutral Hydrogen in Local Group Dwarf Galaxies

    … thesis explores these questions by studying the neutral hydrogen (HI) component of dwarf galaxies. First, limits on the HI mass of the ultra-faint dwarfs are presented, and the HI content of all Local Group dwarf galaxies is examined from an environmental standpoint. We find that those Local …

    columbia-diss Repository record for Neutral Hydrogen in Local Group Dwarf Galaxies (opens in a new tab)

  2. Solar-activity-based neutral hydrogen geocorona model

    Submission published under a 24 month embargo labeled 'U of I Access', the embargo will last until 2024-05-01

    uiuc Repository record for Solar-activity-based neutral hydrogen geocorona model (opens in a new tab)

  3. Neutral hydrogen observations of spiral and irregular galaxies

    This thesis describes hydrogen-line observations using the Cambridge Half-Mile telescope. The initial chapters describe observations of two nearby galaxies af late spiral type, namely M33 and NGC 2403. The severe warping of the HI layer in the outer parts of M33 was clearly seen, and the origin of …

    cambridge Repository record for Neutral hydrogen observations of spiral and irregular galaxies (opens in a new tab)

  4. Compact Galactic Neutral Hydrogen Clouds in the GALFA-HI Survey

    … in our Galaxy appears. Since the detection of neutral hydrogen in 1951, each new survey has revealed new structure. Using the GALFA-HI survey, we have discovered five populations of compact neutral hydrogen clouds. We began by developing a machine-vision algorithm to identify compact clouds in …

    columbia-diss Repository record for Compact Galactic Neutral Hydrogen Clouds in the GALFA-HI Survey (opens in a new tab)

  5. The Omniscope : mapping the Universe in 3D with neutral hydrogen

    21 cm tomography has the potential to become the most powerful cosmological probe yet. The Omniscope is a novel radio telescope being built to take advantage of this signal. This thesis describes my work on integrating, testing, and characterizing all modules of the Omniscope and identifying …

    mit Repository record for The Omniscope : mapping the Universe in 3D with neutral hydrogen (opens in a new tab)

  6. Neutral hydrogen mass distributions in galaxies uncovered by three-dimensional stacking

    Atomic hydrogen (HI) serves as the raw fuel from which the star-forming molecular hydrogen forms - making it an important tracer of galaxy evolution. Due to the intrinsic faintness of the HI emission line (observed at rest at 21 cm), detecting HI emission in galaxies beyond a z = 0.1 becomes …

    cape-town Repository record for Neutral hydrogen mass distributions in galaxies uncovered by three-dimensional stacking (opens in a new tab)

  7. Analysis of low-energy neutral hydrogen fluxes using an electron cyclotron resonance-heated discharge

    … and proof-of-principle verification of a neutral hydrogen flux detection system, based on an ECRH discharge as the neutral flux ionizer. The significant features of the ionizer are its small size and simultaneous excitation of the ECRH mode using a 30 MHz RF driver and relatively small …

    uiuc Repository record for Analysis of low-energy neutral hydrogen fluxes using an electron cyclotron resonance-heated discharge (opens in a new tab)

  8. Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey

    … local universe as the extended distribution of neutral hydrogen makes it susceptible to a wide range of environmental effects that produce peculiar HI morphologies. Moreover, HI enables the study of how galaxies obtain and lose cold gas. The HI distribution of galaxies often exhibits warps, …

    cape-town Repository record for Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey (opens in a new tab)

  9. Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey

    … local universe as the extended distribution of neutral hydrogen makes it susceptible to a wide range of environmental effects that produce peculiar HI morphologies. Moreover, HI enables the study of how galaxies obtain and lose cold gas. The HI distribution of galaxies often exhibits warps, …

    cape-town Repository record for Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey (opens in a new tab)

  10. Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey

    … local universe as the extended distribution of neutral hydrogen makes it susceptible to a wide range of environmental effects that produce peculiar HI morphologies. Moreover, HI enables the study of how galaxies obtain and lose cold gas. The HI distribution of galaxies often exhibits warps, …

    cape-town Repository record for Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey (opens in a new tab)

  11. Quenching mechanisms in recently quenched elliptical galaxies: insights from neutral hydrogen studies and environmental analysis

    … and descendants (postRQEs), focusing on their neutral hydrogen (HI) content and star formation properties. Contrary to conventional quenching models emphasizing gas depletion, RQEs retain substantial HI reservoirs (fgas ≥ 17%), suggesting that quenching is not primarily driven by gas …

    umkc Repository record for Quenching mechanisms in recently quenched elliptical galaxies: insights from neutral hydrogen studies and environmental analysis (opens in a new tab)

  12. Neutral gas and the magnetic field in the Galactic Center

    … via Zeeman splitting of the 21-cm line of neutral hydrogen. In addition, I report a 3$\sigma$ upper limit of 2 mG for $B\sb\Vert$ in the neutral hydrogen within the circumnuclear disk of M82.

    uiuc Repository record for Neutral gas and the magnetic field in the Galactic Center (opens in a new tab)

  13. H (sub) alpha & Neutral Density Scaling in the Maryland Centrifugal eXperiment

    The Maryland Centrifugal eXperiment (MCX) is a hydrogen plasma confinement experiment with a rotating mirror magnetic configuration. This experiment was designed to test the concepts of centrifugal confinement and velocity shear stabilization which may allow scaleability to a fusion reactor. These …

    maryland Repository record for H (sub) alpha & Neutral Density Scaling in the Maryland Centrifugal eXperiment (opens in a new tab)

  14. A HI search for galaxies hidden by the Galactic bulge

    In this thesis, a deep neutral hydrogen (HI) galaxy search for galaxies hidden by the Galactic Bulge is presented. The HI Parkes deep HI Zone of Avoidance (ZOA) survey has been extended towards the higher latitudes in the Galactic Bulge region. The surveyed region covers 332° ≤ l ≤ 36° for the …

    cape-town Repository record for A HI search for galaxies hidden by the Galactic bulge (opens in a new tab)

  15. Studying galaxy formation through Lyman alpha in emission and absorption

    … of the central problems of Physical Cosmology. Neutral hydrogen plays an important role, linking the collapse of cooling gas into haloes with the formation of stars. Lyman alpha, hydrogen’s strongest spectral line, can directly probe neutral hydrogen in the high redshift Universe. Lyα can be …

    cambridge Repository record for Studying galaxy formation through Lyman alpha in emission and absorption (opens in a new tab)

  16. Charge Transfer Cross-Sections for Nitrogen(v) and Sulfur(iii) Ions Interacting With Hydrogen Atoms in Astrophysical Plasmas

    … values for the reactive cross sections involving neutral hydrogen and helium are not generally available. In the absence of such values, one must rely on theoretical calculations of the relevant reaction rates.

    uiuc Repository record for Charge Transfer Cross-Sections for Nitrogen(v) and Sulfur(iii) Ions Interacting With Hydrogen Atoms in Astrophysical Plasmas (opens in a new tab)

  17. Investigating the Epoch of Cosmic Reionisation with Radio Interferometers

    … (EoR) marks the cosmic period during which the neutral hydrogen (H I) that pervaded the Universe transitioned to an almost entirely ionised state. This process was driven by the energetic photons emitted by the first luminous sources. As such, the EoR encodes crucial information about the nature …

    cambridge Repository record for Investigating the Epoch of Cosmic Reionisation with Radio Interferometers (opens in a new tab)

  18. Illuminating the Universe : New Probes of Reionization and Cosmology

    We model the epoch of hydrogen reionisation of the universe, using analytic as well as numerical methods. In a detailed statistical analysis of our results, we find good agreement in the alternative descriptions of the morphology of ionized regions. We use the simulations to make predictions for …

    heid-diss Repository record for Illuminating the Universe : New Probes of Reionization and Cosmology (opens in a new tab)

  19. Robust Estimation Techniques for the Cosmological Analysis of Large Scale Structure

    … counts-in-cells statistic for the first time to neutral hydrogen. Neutral hydrogen is particularly interesting for counts-in-cells statistics because of the vast regions that can be covered by intensity mapping. We find percent-level accuracy when comparing the prediction for the density in …

    cambridge Repository record for Robust Estimation Techniques for the Cosmological Analysis of Large Scale Structure (opens in a new tab)

  20. A multi-wavelength study of the dwarf galaxies NGC 2915 and NGC 1705 : star formation, gas dynamics and dark matter

    … each galaxy consists of new observations of the neutral hydrogen (Hi) line obtained with the Australia Telescope Compact Array, October 2006 - May 2007. The stellar disk of NGC 1705 is host to an intense star-bursting core which is rapidly depleting the galaxy's central Hi reservoir. This galaxy …

    cape-town Repository record for A multi-wavelength study of the dwarf galaxies NGC 2915 and NGC 1705 : star formation, gas dynamics and dark matter (opens in a new tab)

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