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Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5

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    0518288 - ASÚ 2020 RIV US eng J - Journal Article
    Luo, Y. - Németh, Péter - Deng, L. - Han, Z.
    Hot Subdwarf Stars Observed in Gaia DR2 and LAMOST DR5.
    Astrophysical Journal. Roč. 881, č. 1 (2019), č. článku 7. ISSN 0004-637X. E-ISSN 1538-4357
    R&D Projects: GA ČR(CZ) GA18-20083S
    Institutional support: RVO:67985815
    Keywords : kinematics and dynamics * subdwarfs * surveys
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 5.746, year: 2019
    Method of publishing: Limited access
    https://doi.org/10.3847/1538-4357/ab298d

    Combing Gaia DR2 with LAMOST DR5, we spectroscopically identified 924 hot subdwarf stars, among which 32 stars exhibit strong double-lined composite spectra. We measured the effective temperature T-eff, surface gravity logg, helium abundance y = nHe/nH, and radial velocities of 892 non-composite spectra hot subdwarf stars by fitting LAMOST observations with Tlusty/Synspec non-LTE synthetic spectra. We outlined four different groups in the T-eff-logg diagram with our helium abundance classification scheme and two nearly parallel sequences in the T-eff-log(y) diagram.
    Permanent Link: http://hdl.handle.net/11104/0303445

     
     
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