Results 111 to 120 of about 20,344 (216)

Two Long-period Giant Planets around Two Giant Stars: HD 112570 and HD 154391

open access: yesThe Astronomical Journal
We present the discoveries of two giant plants orbiting the red-giant-branch star HD 112570 and the red-clump star HD 154391, based on the radial-velocity (RV) measurements from the Xinglong station and Okayama Astrophysical Observatory.
Guang-Yao Xiao   +26 more
doaj   +1 more source

Asteroseismology of 687 TESS Red Giants: Individual Frequencies and Asymptotic Parameters

open access: yesThe Astrophysical Journal Supplement Series
The individual modes and asymptotic parameters are important characteristics of stellar oscillation. Using TESS 2 minute cadence data from Sectors 1 to 75, we perform asteroseismic analysis of 687 red giants, and provide their oscillation mode parameters.
Jianzhao Zhou   +10 more
doaj   +1 more source

Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts

open access: yesThe Astrophysical Journal
Asteroseismology has emerged as a powerful tool to unravel the intricate relationships between evolved stars and their planetary systems. In this study, we leverage this technique to investigate the evolutionary stages of five exoplanet host stars, each ...
Wen-Xu Lin   +7 more
doaj   +1 more source

The Structure, Populations, and Kinematics of the Milky Way Central and Inner Bulge with OGLE, APOGEE, and Gaia Data

open access: yesThe Astrophysical Journal
We present an analysis of the structure, kinematics, and chemo-dynamical properties of the Milky Way bulge using RR Lyrae stars from Optical Gravitational Lensing Experiment (OGLE), and giant stars from APOGEE and Gaia that have distances placing them in
Xiao Han   +7 more
doaj   +1 more source

The Spectroscopic Disambiguation of the Red Clump from the Red Giant Branch

open access: yes
This thesis delves into the spectro-seismic connection observed in red giant stars, affirming that the necessary asteroseismic information for effectively discerning standard-candle red clump stars (RC) from non-standard-candle red giant branch (RGB) stars is embedded within their spectra.
openaire   +2 more sources

Unraveling the Kinematic and Morphological Evolution of the Small Magellanic Cloud

open access: yesThe Astrophysical Journal
We model the kinematics of the Small Magellanic Cloud (SMC) by analyzing the proper motions (PMs) from Gaia DR3 of nine different stellar populations, including young main-sequence (MS) stars (
S. R. Dhanush   +2 more
doaj   +1 more source

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