Search Publications

Direct-imaging Discovery and Dynamical Mass of a Substellar Companion Orbiting an Accelerating Hyades Sun-like Star with SCExAO/CHARIS
DOI: 10.3847/2041-8213/ac772f Bibcode: 2022ApJ...934L..18K

Currie, Thayne; Kwon, Jungmi; Tamura, Motohide +33 more

We present the direct-imaging discovery of a substellar companion in orbit around a Sun-like star member of the Hyades open cluster. So far, no other substellar companions have been unambiguously confirmed via direct imaging around main-sequence stars in Hyades. The star HIP 21152 is an accelerating star as identified by the astrometry from the Ga…

2022 The Astrophysical Journal
Gaia Hipparcos 41
RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
DOI: 10.3847/1538-4357/ac69e6 Bibcode: 2022ApJ...932...19N

El-Badry, Kareem; Weisz, Daniel R.; Nagarajan, Pranav

We provide uniform RR Lyrae-based distances to 39 dwarf galaxies in and around the Local Group. We determine distances based on a Bayesian hierarchical model that uses periods and magnitudes of published RR Lyrae in dwarf galaxies and is anchored to well-studied Milky Way (MW) RR Lyrae with spectroscopic metallicities and Gaia eDR3 parallaxes. Gai…

2022 The Astrophysical Journal
Gaia Hipparcos eHST 20
Dynamical Masses of the Primary Be Star and Secondary sdB Star in the Single-lined Binary κ Dra (B6 IIIe)
DOI: 10.3847/1538-4357/ac98b8 Bibcode: 2022ApJ...940...86K

Gies, Douglas R.; Wang, Luqian; Klement, Robert +16 more

Because many classical Be stars may owe their nature to mass and angular-momentum transfer in a close binary, the present masses, temperatures, and radii of their components are of high interest for comparison to stellar evolution models. Object κ Dra is a 61.5 day single-lined binary with a B6 IIIe primary. With the CHARA Array instruments MIRC/M…

2022 The Astrophysical Journal
AKARI Gaia Hipparcos IUE 17
The Orbits and Dynamical Masses of the Castor System
DOI: 10.3847/1538-4357/ac9d8d Bibcode: 2022ApJ...941....8T

Torres, Guillermo; Klement, Robert; Monnier, John D. +12 more

Castor is a system of six stars in which the two brighter objects, Castor A and B, revolve around each other every ~450 yr and are both short-period spectroscopic binaries. They are attended by the more distant Castor C, which is also a binary. Here we report interferometric observations with the Center for High Angular Resolution Astronomy (CHARA…

2022 The Astrophysical Journal
Gaia Hipparcos 4