Focal Interest
Focal Interest

Astro and Planetary Science

External reference: https://openalex.org/T10325

  1. Mars clay-bearing rocks yielded more than 20 organic molecules
  2. DM Tau disk shows non-thermal line broadening
    Bayesian analysis of molecular line observations confirms nonthermal broadening of 0.4 sound speeds in the DM Tau protoplanetary disk, providing evidence for turbulence.
  3. Frame center acceleration method was more consistent in trajectory modeling
    Compare orbital perturbation modeling methods using ephemeris data. Analyze indirect and frame center acceleration approaches for Earth-Moon system trajectories, examining consistency versus.
  4. Tomographic line analysis identifies possible embedded planets in disks
    Tomographic analysis of molecular line observations enables detection of embedded planets in protoplanetary disks, revealing multiple planet candidates in HD 135344B and MWC 758.
  5. Large protoplanetary disks show widespread non-Keplerian gas motions
    Two-dimensional kinematic mapping of 15 protoplanetary disks reveals ubiquitous non-Keplerian deviations including spiral structures, with systematic differences between disk classifications.