Results 31 to 40 of about 4,112,115 (294)

Quantifying Uncertainties on the Tip of the Red Giant Branch Method

open access: yesThe Astronomical Journal, 2023
We present an extensive grid of numerical simulations quantifying the uncertainties in measurements of the tip of the red giant branch (TRGB). These simulations incorporate a luminosity function composed of 2 mag of red giant branch (RGB) stars leading ...
Barry F. Madore   +3 more
doaj   +1 more source

Ensemble asteroseismology of red-giant stars

open access: yes, 2011
The successful launches of the CoRoT and Kepler space missions have led to the detections of solar-like oscillations in large samples of red-giant stars. The large numbers of red giants with observed oscillations make it possible to investigate the properties of the sample as a whole: ensemble asteroseismology.
Hekker, S.   +5 more
openaire   +3 more sources

Red Giant evolution and specific problems [PDF]

open access: yes, 2013
In spite of the great effort made in the last decades to improve our understanding of stellar evolution, significant uncertainties still remain due to our poor knowledge of some complex physical processes that still require an empirical calibration, such
Girardi, L.   +17 more
core   +1 more source

Irregular Red-Giant Variable Stars [PDF]

open access: yesInternational Astronomical Union Colloquium, 1989
Aperiodic intrinsic variability becomes increasingly evident for a greater number of red giant and supergiant stars as observations become more technically refined and extended over a longer time. All red variables show an erratic temporal behavior to some degree.
M. Querci, F. Querci
openaire   +1 more source

Modelling of Red Giant Stars: The state-of-the-art [PDF]

open access: yes, 2017
The seismic data obtained by the CoRoT and Kepler space missions have provided inferences of the global and structural properties of thousands of red giants.
CASSISI, Santi   +2 more
core   +1 more source

Red-Giant Stars With Low Period Spacings

open access: yes, 2022
The ability of studying the interior structure of stars makes asteroseismology a powerful method to learn more about stars. Additionally, the large amount of data provided by space telescopes like Kepler makes it possible to observe stars in short ...
Braun, Teresa A. M.
core   +1 more source

Harlow Shapley and Red Giant Stars [PDF]

open access: yesSymposium - International Astronomical Union, 1988
In five papers written between 1951 and 1955 Shapley considers the topic of red giant stars and reddish variable stars in the Magellanic Clouds. These works coincide with Shapley's final year as Director at Harvard and the first years of his retirement which extended a full score of years before his death in 1972. They include the following: Magellanic
F. Martin, S. J. McCarthy
openaire   +1 more source

Asteroseismic inferences from red-giant stars [PDF]

open access: yes, 2018
The analysis of high-precision long-term photometric time-series of data from the NASA Kepler space mission (2008 − 2012) has revolutionized the field of red-giant seismology.
Themeẞl, Nathalie
core   +1 more source

Ensemble Asteroseismology of Red-giant Stars [PDF]

open access: yes, 2012
The successful launches of the CoRoT and Kepler space missions have led to the detections of solar-like oscillations in large samples of red-giant stars.
De Ridder, J.   +5 more
core   +5 more sources

Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS [PDF]

open access: yes, 2021
We report the discovery of planetary companions orbiting four low-luminosity giant stars with M⋆ between 1.04 and 1.39 M⊙. All four host stars have been independently observed by the EXoPlanets aRound Evolved StarS (EXPRESS) program and the Pan-Pacific ...
Wittenmyer, R.   +33 more
core   +1 more source

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