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Radio/X-ray correlations and variability in the X-ray binary LS I +61°303
R. Sharma, M. Massi, M. Chernyakova +6
The high-mass X-ray binary LS I +61°303 exhibits variability in its radio and X-ray emissions, ranging from minute to hour time-scales. At such short time-scales, not much is known…
Evidence for periodic accretion-ejection in LSI+61303
M. Massi, M. Chernyakova, A. Kraus +7
The stellar binary system LS I +61303, composed of a compact object in an eccentric orbit around a B0 Ve star, emits from radio up to gamma-ray energies. The orbital modulation of…
When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147
Jason Lee Curtis, Marcel A. Agüeros, Sean P. Matt +17
Recent measurements of rotation periods () in the benchmark open clusters Praesepe (670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after convergi…
ACRONYM IV: Three New, Young, Low-mass Spectroscopic Binaries
Laura Flagg, Evgenya L. Shkolnik, Alycia Weinberger +4
As part of our search for new low-mass members of nearby young moving groups (YMG), we discovered three low-mass, spectroscopic binaries, two of which are not kinematically associa…
Dynamical masses for the Pleiades binary system HII-2147
Guillermo Torres, Carl Melis, Adam L. Kraus +3
We report our long-term spectroscopic monitoring of the Pleiades member HII-2147, which has previously been spatially resolved at radio wavelengths in VLBI observations. It has als…
TESS Hunt for Young and Maturing Exoplanets (THYME) II: A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association
Aaron C. Rizzuto, Elisabeth R. Newton, Andrew W. Mann +10
We present the discovery of a transiting hot Jupiter orbiting HIP 67522 ( K; ) in the 10-20 Myr old Sco-Cen OB association. We identified t…