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astro-ph.SR2024
Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 127
Dane Spaeth, Sabine Reffert, Emily L. Hunt +2
Several evolved stars have been found to exhibit long-period radial velocity variations that cannot be explained by planetary or brown dwarf companions. Non-radial oscillations cau…
astro-ph.GA2024
Most nearby young star clusters formed in three massive complexes
Cameren Swiggum, João Alves, Robert Benjamin +9
Efforts to unveil the structure of the local interstellar medium and its recent star formation history have spanned the past seventy years. Recent studies utilizing precise data fr…