Results 1 to 10 of about 114 (114)

A Catalog of Nearby Accelerating Star Candidates in Gaia DR3

open access: yesThe Astronomical Journal, 2023
We describe a new catalog of accelerating star candidates with Gaia G ≤ 17.5 mag and distances d ≤ 100 pc. Designated as the Gaia Nearby Accelerating Star Catalog (GNASC), it contains 29,684 members identified using a supervised machine-learning ...
Marc L. Whiting   +3 more
doaj   +1 more source

Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?

open access: yesThe Astrophysical Journal, 2022
In this paper, we report the potential detection of a nonmonotonic radial rotation profile in a low-mass lower-luminosity giant star. For most low- and intermediate-mass stars, the rotation on the main sequence seems to be close to rigid.
Jamie Tayar   +17 more
doaj   +1 more source

Direct Imaging Explorations for Companions around Mid–Late M Stars from the Subaru/IRD Strategic Program

open access: yesThe Astronomical Journal, 2023
The Subaru telescope is currently performing a strategic program (SSP) using the high-precision near-infrared (NIR) spectrometer IRD to search for exoplanets around nearby mid/late M dwarfs via radial velocity (RV) monitoring.
Taichi Uyama   +34 more
doaj   +1 more source

Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-dwarf Companion in the Hyades

open access: yesThe Astronomical Journal, 2023
Benchmark brown dwarf companions with well-determined ages and model-independent masses are powerful tools to test substellar evolutionary models and probe the formation of giant planets and brown dwarfs.
Kyle Franson   +30 more
doaj   +1 more source

Verification of Gaia Data Release 3 Single-lined Spectroscopic Binary Solutions With Three Transiting Low-mass Secondaries

open access: yesThe Astronomical Journal, 2023
While secondary mass inferences based on single-lined spectroscopic binary (SB1) solutions are subject to $\sin i$ degeneracies, this degeneracy can be lifted through the observations of eclipses.
Stephen P. Schmidt   +20 more
doaj   +1 more source

Statistics on the population of distant substellar companions to nearby stars

open access: yesAstronomy & Astrophysics
Context. Wide substellar companions to stars provide valuable benchmarks for investigating the formation and evolutionary pathways of brown dwarfs and giant planets far beyond the extent of protoplanetary discs.
Ouedraogo Souleymane   +7 more
doaj   +1 more source

Predicted incidence of Jupiter-like planets around white dwarfs

open access: yesAstronomy & Astrophysics
Context. Gas-giant planets and brown dwarfs have been discovered in large numbers around main-sequence stars and even evolved stars. In contrast, and despite ongoing imaging surveys using state-of-the-art facilities, only a handful of substellar ...
Mauch-Soriano Alex   +9 more
doaj   +1 more source

Testing the Interaction between a Substellar Companion and a Debris Disk in the HR 2562 System

open access: yesThe Astronomical Journal, 2023
The HR 2562 system is a rare case where a brown dwarf companion resides in a cleared inner hole of a debris disk, offering invaluable opportunities to study the dynamical interaction between a substellar companion and a dusty disk.
Stella Yimiao Zhang   +53 more
doaj   +1 more source

Apache Point Observatory Follow-up of ACcelerating Candidate ExopLanet Host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere

open access: yesThe Astronomical Journal
Directly imaged substellar companions with well-constrained ages and masses serve as vital empirical benchmarks for planet formation and evolution models. Potential benchmark companions can be identified from astrometric accelerations of their host stars.
Anne E. Peck   +16 more
doaj   +1 more source

JWST/NIRSpec Observations of the Planetary Mass Companion TWA 27B

open access: yesThe Astrophysical Journal Letters, 2023
We present 1–5 μ m spectroscopy of the young planetary mass companion TWA 27B (2M1207B) performed with NIRSpec on board the James Webb Space Telescope. In these data, the fundamental band of CH _4 is absent, and the fundamental band of CO is weak.
K. L. Luhman   +10 more
doaj   +1 more source

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