Global ETD Search

Search theses and dissertations gathered from participating repositories worldwide. Every result links back to the library that holds it. No account is needed.

Results

Showing 1 to 6 of 6 for “"Herbig Ae/Be stars"”.

  1. Parameterizing the Dust Around Herbig Ae/Be Stars: Multiwavelength Imaging, Radiative Transfer Modeling, and Near-Infrared Instrumentation

    … capabilities available for observations of Herbig Ae/Be stars, I have participated in the development of the WIYN High Resolution Infrared Camera. The instrument operates in the near-infrared (∼0.8 -- 2.5 mum), includes 13 filters, and has a pixel size of ∼0.1&inches;, resulting in a …

    uiuc Repository record for Parameterizing the Dust Around Herbig Ae/Be Stars: Multiwavelength Imaging, Radiative Transfer Modeling, and Near-Infrared Instrumentation (opens in a new tab)

  2. Understanding the Star -Forming Environment in Stellar Clusters

    … for the formation of low-mass cluster members. Embedded, young, and intermediate-mass stellar clusters around Herbig Ae/Be stars are sampled. Mid- and near-infrared observations identifying young stars and millimeter interferometric observations probing dense molecular gas and dust …

    uiuc Repository record for Understanding the Star -Forming Environment in Stellar Clusters (opens in a new tab)

  3. Photometric monitoring of early type emission line stars

    … MNQ) photometry of early type, emission line, stars is described. Particular emphasis is placed on observations of suspected pre-main-sequence objects such as Herbig Ae/Be stars. The observations, together with data from the IRAS point source catalogue, are analysed to probe the circumstellar …

    cent-lancashire Repository record for Photometric monitoring of early type emission line stars (opens in a new tab)

  4. High resolution studies of early type emission line stars

    … is used to separate the spectra of unresolved Herbig Ae/Be binary systems. The separated spectra allow the mass ratio of the systems to be established. The separation and mass ratio distribution of the systems suggest that they form via disk fragmentation. To test this conclusion, disk and …

    whiterose Repository record for High resolution studies of early type emission line stars (opens in a new tab)

  5. The Inner Gaseous Disks Of Herbig Be Stars

    Herbig Ae/Be stars are intermediate mass (~2 to 20Msun) pre-main sequence stars that inherit a circumstellar disk of dust and gas from their formation phase. The region of this disk closest to the star is entirely gaseous because dust evaporates at the high temperatures there, and this gaseous …

    uwo Repository record for The Inner Gaseous Disks Of Herbig Be Stars (opens in a new tab)