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Advanced filters: Author: Shubham Kanodia Clear advanced filters

  • The spectroscopic and photometric observations of a high-mass, transiting warm Jupiter, TIC 241249530 b, with an orbital eccentricity of 0.94, provide evidence that hot Jupiters may have formed by means of a high-eccentricity tidal-migration pathway.

    • Arvind F. Gupta
    • Sarah C. Millholland
    • Carl Ziegler
    ResearchOpen Access
    Nature
    Volume: 632, P: 50-54