Showing 21 - 29 results of 29 for search '"chemically peculiar star"', query time: 0.80s Refine Results
  1. 21
    The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis

    The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis by Zachary Reeves, Kevin C. Schlaufman, Henrique Reggiani

    Published 2023-01-01
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  2. 22
    The Carbon Star DY Persei May Be a Cool R Coronae Borealis Variable

    The Carbon Star DY Persei May Be a Cool R Coronae Borealis Variable by D. A. García-Hernández, N. Kameswara Rao, David L. Lambert, K. Eriksson, A. B. S. Reddy, Thomas Masseron

    Published 2023-01-01
    Subjects: “…Chemically peculiar stars…”
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  3. 23
    Iron-rich Metal-poor Stars and the Astrophysics of Thermonuclear Events Observationally Classified as Type Ia Supernovae. I. Establishing the Connection

    Iron-rich Metal-poor Stars and the Astrophysics of Thermonuclear Events Observationally Classified as Type Ia Supernovae. I. Establishing the Connection by Henrique Reggiani, Kevin C. Schlaufman, Andrew R. Casey

    Published 2023-01-01
    Subjects: “…Chemically peculiar stars…”
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  4. 24
    HST spectroscopy of chemically peculiar hot subdwarfs: PG 0909+276 and UVO0512–08

    HST spectroscopy of chemically peculiar hot subdwarfs: PG 0909+276 and UVO0512–08 by Wild James, Jeffery Christopher Simon

    Published 2017-12-01
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  5. 25
    Binary Central Stars of Planetary Nebulae

    Binary Central Stars of Planetary Nebulae by David Jones

    Published 2020-04-01
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  6. 26
    CHEMICAL COMPOSITION OF PECULIAR STAR HD91375 – THE MEMBER OF SIRIUS MOVING GROUP

    CHEMICAL COMPOSITION OF PECULIAR STAR HD91375 – THE MEMBER OF SIRIUS MOVING GROUP by V. Yushchenko

    Published 2009-12-01
    “…We present the results of determinations of the abundances of chemical elements in the atmosphere of hot chemically peculiar star HD91375 – member of Sirius moving group. …”
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  7. 27
    Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method: I

    Searching for Barium Stars from the LAMOST Spectra Using the Machine-learning Method: I by Fengyue Guo, Zhongding Cheng, Xiaoming Kong, Yatao Zhang, Yude Bu, Zhenping Yi, Bing Du, Jingchang Pan

    Published 2023-01-01
    “…Barium stars are chemically peculiar stars that exhibit enhancement of s -process elements. …”
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  8. 28
    Diffusion in hot subdwarf progenitors from the common envelope channel

    Diffusion in hot subdwarf progenitors from the common envelope channel by Byrne Conor M., Jeffery C. Simon, Tout Christopher A., Hu Haili

    Published 2017-12-01
    “…Diffusion of elements in the atmosphere of a star can drastically affect its surface composition, sometimes leading to unusual mixtures. These chemically peculiar stars can be identified fromthe presence of unusual lines in their spectra. …”
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  9. 29
    MAGNETIZATION OF STARS VS. THE EFFECTIVE TEMPERATURE

    MAGNETIZATION OF STARS VS. THE EFFECTIVE TEMPERATURE by V. D. Bychkov, L. V. Bychkova, J. Madej

    Published 2008-12-01
    “…At the same time chemically peculiar stars neatly block to the two groups: "weak" - magnetic (Am and Hg-Mn stars) and "strong" - magnetic (SrCrEu, Sr, Si, He-w and He-r stars). …”
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