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Showing 1 to 4 of 4 for “"Combined Array for Research in Millimeter-wave Astronomy (CARMA)"”.

  1. Gas distribution, star formation and giant molecular cloud evolution in nearby spiral galaxies

    In this thesis, I present a detailed study of the resolved properties of the cold gas in nearby galaxies at different size scales, starting from the whole galactic disk to the size of the Giant Molecular Clouds (GMCs). Differences in the shape and width of global CO and HI spectra of resolved disks …

    uiuc Repository record for Gas distribution, star formation and giant molecular cloud evolution in nearby spiral galaxies (opens in a new tab)

  2. Understanding star formation at early stages in the filamentary era

    This thesis presents a study of star formation at early stages in the filamentary era with a special focus on massive star and cluster formation. We first investigate the importance of filamentary structures in star formation and propose an observationally driven scenario for the evolution of …

    uiuc Repository record for Understanding star formation at early stages in the filamentary era (opens in a new tab)

  3. Circumstellar Structure Properties of Young Stellar Objects: Envelopes, Bipolar Outflows, and Disks

    Physical properties of the three main structures in young stellar objects (YSOs), envelopes, bipolar outflows, and circumstellar disks, have been studied using radio interferometers: the Berkeley-Illinois-Maryland Association (BIMA) array and the Combined Array for Research in Millimeter-wave

    uiuc Repository record for Circumstellar Structure Properties of Young Stellar Objects: Envelopes, Bipolar Outflows, and Disks (opens in a new tab)

  4. Observations of disks around the youngest protostars: Characterizing frequency, dust properties, and magnetic fields at the earliest times

    Circumstellar disks are fundamental for accretion and angular momentum distribution during the early phases of star formation. Class 0 objects are the youngest protostars and most embedded in their natal envelopes, and circumstellar disks can form even at this earliest stage of star formation. …

    uiuc Repository record for Observations of disks around the youngest protostars: Characterizing frequency, dust properties, and magnetic fields at the earliest times (opens in a new tab)