Two Long-period Giant Planets around Two Giant Stars: HD 112570 and HD 154391
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
Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS II. Deciphering Gaia parallax systematics using red clump stars [PDF]
S. Khan +4 more
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Asteroseismology of 687 TESS Red Giants: Individual Frequencies and Asymptotic Parameters
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
The morphology of the sub-giant branch and red clump reveal no sign of age spreads in intermediate-age clusters [PDF]
N. Bastian, Florian Niederhofer
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Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts
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
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 complete chloroplast genome of Fargesia angustissima T. P. Yi: a panda dietary bamboo species. [PDF]
Wu H, Li X, Xu X, Zhang Y, Su T.
europepmc +1 more source
The Spectroscopic Disambiguation of the Red Clump from the Red Giant Branch
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
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
Parameters of the local warp of the stellar-gaseous galactic disk from the kinematics of Tycho-2 nearby red giant clump stars [PDF]
В. В. Бобылев
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