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Showing 1 to 7 of 7 for “"Yso"”.

  1. The Evolution of Massive Young Stellar Objects in the Large Magellanic Cloud

    … analysis. Using this analysis, we classify the YSO spectra into several distinct groups based upon their dominant spectral features: silicate absorption (S Group), silicate absorption and fine-structure line emission (SE), polycyclic aromatic hydrocarbon (PAH) emission (P Group), PAH and …

    uiuc Repository record for The Evolution of Massive Young Stellar Objects in the Large Magellanic Cloud (opens in a new tab)

  2. Modelling Of Protostellar Jets Using Intense Lasers

    … learning about the effects of these factors on YSO jets by studying their scaled laboratory counterparts. The second experiment was designed to be similar to the first in order to investigate applying the scaling relations to scaling between laboratory experiments. Previous work in this area has …

    whiterose Repository record for Modelling Of Protostellar Jets Using Intense Lasers (opens in a new tab)

  3. Understanding the Earliest Stages of High-mass Star Formation

    … an analysis of the young stellar objects (YSO), the regions currently hosting on-going high-mass star formation, the environment, history, and compact source population. Spitzer data were used to identify, classify, and investigate the clustering properties of the YSO population. These …

    toronto-retro Repository record for Understanding the Earliest Stages of High-mass Star Formation (opens in a new tab)

  4. The characterization of volatiles associated with young stellar objects

    … respectively, toward 28 Young Stellar Objects (YSOs). We found that more than 50% of the YSOs studied contained a portion of crystalline CO₂ ice. We also found that some sources with Flat or borderline Class II Spectral Energy Distributions (SEDs) have a larger abundance of CO₂ ice with respect …

    must-thes Repository record for The characterization of volatiles associated with young stellar objects (opens in a new tab)

  5. The environmental impact of high- and low-mass stars: from formation to main sequence

    … regions around massive young stellar objects (YSOs) and explore numerous relationship between parameters measured through observations of free-free and infrared emission. In particular, we find that YSO mass is a crucial consideration when exploring almost any relationship. Finally, we analyze …

    uiuc Repository record for The environmental impact of high- and low-mass stars: from formation to main sequence (opens in a new tab)

  6. The morphology and kinematics of star forming regions

    … clumps, following an arc equidistant from the YSO, suggest that the outflow is precessing. This work concludes with the first coupled gas-solid maps. This thesis demonstrates the importance of understanding the often complex morphology and kinematics of a star forming region prior to …

    strathclyde Repository record for The morphology and kinematics of star forming regions (opens in a new tab)

  7. Observations of protostellar systems across sub/millimeter wavelengths in nearby molecular clouds

    Submission original under an indefinite embargo labeled 'Open Access'. The submission was exported from vireo on 2025-03-28 without embargo terms

    uiuc Repository record for Observations of protostellar systems across sub/millimeter wavelengths in nearby molecular clouds (opens in a new tab)