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pro vyhledávání: '"Schussler, Joshua A"'
In this project, we determined the constraints on the modified tidal quality factor, $Q_{pl}'$, of gas-giant planets orbiting close to their host stars. We allowed $Q_{pl}'$ to depend on tidal frequency, accounting for the multiple tidal waves with t
Externí odkaz:
http://arxiv.org/abs/2308.06324
Publikováno v:
Monthly Notices of the Royal Astronomical Society, p.stad2194 (2023)
Tidal dissipation in binary systems is the primary source for synchronization and circularization of the objects in the system. The efficiency of the dissipation of tidal energy inside stars or planets results in significant changes in observed prope
Externí odkaz:
http://arxiv.org/abs/2307.13074
Publikováno v:
Monthly Notices of the Royal Astronomical Society 2022, stac2618
Tidal friction has long been recognized to circularize the orbits of binary stars over time. In this study, we use the observed distribution of orbital eccentricities in populations of binary stars to probe tidal dissipation. In contrast to previous
Externí odkaz:
http://arxiv.org/abs/2209.08109
Autor:
Schussler, Joshua Aaron
That there is a mismatch between the observed mass of galaxies and their resulting motion has been known for decades. One explanation for this discrepancy, Modified Newtonian Dynamics, or MOND, presents many exciting avenues of exploration. In partic
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 10/15/2023, Vol. 525 Issue 1, p876-897, 22p
Auxiliary data associated with the article "Constraints on Tidal Quality Factor in Kepler Eclipsing Binaries using Tidal Synchronization: A Frequency-Dependent Approach" by Patel, R., Penev, K. and Schussler J. The contents of the files are as follow
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1809008b11c0ecf27b5f6a280e095d25