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The Debiased Compositional Distribution of MITHNEOS: Global Match between the Near-Earth and Main-belt Asteroid Populations, and Excess of D-type Near-Earth Objects
DOI: 10.3847/1538-3881/ac532f Bibcode: 2022AJ....163..165M

Granvik, Mikael; Carry, Benoit; Marsset, Michaël +10 more

We report 491 new near-infrared spectroscopic measurements of 420 near-Earth objects (NEOs) collected on the NASA InfraRed Telescope Facility as part of the MIT-Hawaii NEO Spectroscopic Survey. These measurements were combined with previously published data from Binzel et al. and bias-corrected to derive the intrinsic compositional distribution of…

2022 The Astronomical Journal
AKARI 29
Rotation of Low-mass Stars in Upper Centaurus-Lupus and Lower Centaurus-Crux with TESS
DOI: 10.3847/1538-3881/ac75f1 Bibcode: 2022AJ....164...80R

Powell, Brian P.; Kruse, Ethan; Rebull, L. M. +3 more

We present stellar rotation rates derived from Transiting Exoplanet Survey Satellite (TESS) light curves for stars in Upper Centaurus-Lupus (UCL; ~136 pc, ~16 Myr) and Lower Centaurus-Crux (LCC; ~115 pc, ~17 Myr). We find spot-modulated periods (P) for ~90% of members. The range of light-curve and periodogram shapes echoes that found for other clu…

2022 The Astronomical Journal
AKARI Gaia 20
A Gaia View on the Star Formation in the Monoceros OB1 and R1 Associations
DOI: 10.3847/1538-3881/ac63b6 Bibcode: 2022AJ....163..266L

Lim, Beomdu; Lee, Jeong-Eun; Park, Byeong-Gon +5 more

Stellar kinematics provides the key to understanding the star formation process. In this respect, we present a kinematic study of the Monoceros OB1 (Mon OB1) and R1 (Mon R1) associations using the recent Gaia data and radial velocities of stars derived from high-resolution spectroscopy and the literature. A total of 728 members are selected using …

2022 The Astronomical Journal
AKARI Gaia 13
The Interferometric Binary ϵ Cnc in Praesepe: Precise Masses and Age
DOI: 10.3847/1538-3881/ac7329 Bibcode: 2022AJ....164...34M

Klement, Robert; Monnier, John D.; Schaefer, Gail H. +16 more

We observe the brightest member of the Praesepe cluster, ϵ Cnc, to precisely measure the characteristics of the stars in this binary system, en route to a new measurement of the cluster's age. We present spectroscopic radial velocity measurements and interferometric observations of the sky-projected orbit to derive the masses, which we find to be …

2022 The Astronomical Journal
AKARI Gaia 4