11 research outputs found

    A Neural Network Approach to Identifying YSOs and Exploring Solar Neighborhood Star-Forming History

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    Stellar ages can act as a marker of birth cluster membership for young stellar objects (YSOs), which allows for an improved understanding of the history of star formation in the solar neighborhood. However, the ages of YSOs have historically been difficult to predict on a large scale. Here, we develop a system of convolution neural network models to differentiate between YSOs and their more-evolved counterparts and predict YSO ages using Gaia and 2MASS photometry. The full model and resulting catalog recovers the properties of well-studied young stellar populations to a distance of five kiloparsecs, with significantly higher sensitivity within one kiloparsec, while also identifying new YSO candidate stars. We then explore the resulting catalog\u27s implications for solar neighborhood star formation, and identify several large-scale structures, including two interesting ring or bubble-shaped groupings of young stars which may suggest radially triggered star forming events. Our results support the existence of an inclined Gould\u27s Belt of local star formation, which may coincide with the Local Bubble. In addition, we also identify 26 high velocity \u27runaway\u27 stars from the Orion Nebula Cluster and characterize their likely origins

    Predicting Young Stellar Ages with Deep Learning

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    Studying the environments of star forming regions is critical to our understanding of early stellar evolution, but historically, observationally distinguishing clustered young stars from evolved field stars has been difficult. The ESA’s Gaia telescope allows for vastly improved cluster membership constraints through spatial and kinematical groupings, but this method fails for gravitationally ejected or high velocity members. Stellar ages, which can be extrapolated on an individual basis from photometric measurements, are a more general alternative to astrometric clustering in identifying cluster membership. We present a deep learning method using Gaia and 2MASS photometry to predict stellar ages for the pre-main-sequence branch. Our model, consisting of two cascading neural networks, is trained to recognize young stars and stellar ages derived from the cluster isochrone fitting of nearby star forming regions. After classifying the evolutionary stage of input stars, the model predicts ages for all sources categorized as pre-main-sequence. Our model successfully recovers known nearby star forming regions while identifying additional candidate members from the Gaia catalog, and shows promise for use in studying extreme stellar kinematics in these regions
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