Results 1 to 10 of about 96,030 (294)

Stellar ages from asteroseismology [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
Asteroseismology provides powerful means to probe stellar interiors. The oscillations frequencies are closely related to stellar interior properties via the density and sound speed profiles.
Aizenman   +17 more
core   +3 more sources

Towards age/rotation/magnetic activity relation with seismology

open access: yesEPJ Web of Conferences, 2015
The knowledge of stellar ages directly impacts the characterization of a planetary system as it puts strong constraints on the moment when the system was born. Unfortunately, the determination of precise stellar ages is a very difficult task.
Mathur Savita
doaj   +3 more sources

Magnetic Activity Evolution of Solar-like Stars. I. S ph–Age Relation Derived from Kepler Observations

open access: yesThe Astrophysical Journal, 2023
The ages of solar-like stars have been at the center of many studies such as exoplanet characterization or Galactic-archeology. While ages are usually computed from stellar evolution models, relations linking ages to other stellar properties, such as ...
Savita Mathur   +11 more
doaj   +1 more source

Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution

open access: yesThe Astrophysical Journal, 2023
Stellar ages are key for determining the formation history of the Milky Way, but are difficult to measure precisely. Furthermore, methods that use chemical abundances to infer ages may entangle the intrinsic evolution of stars with the chemodynamical ...
Jeff Shen   +4 more
doaj   +1 more source

Cosmological Constant from Boundary Condition and Its Implications beyond the Standard Model

open access: yesUniverse, 2023
Standard cosmology has long been plagued by a number of persistent problems. The origin of the apparent acceleration of the cosmic expansion remains enigmatic.
Jan O. Stenflo
doaj   +1 more source

Living with a Red Dwarf: X-Ray, UV, and Ca ii Activity–Age Relationships of M Dwarfs

open access: yesThe Astrophysical Journal, 2023
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and luminosities result in slow rates of nuclear evolution and minimal changes to the stars’ observable properties, even along astronomical timescales.
Scott G. Engle
doaj   +1 more source

The Abundance of S-Process Elements: Temporal and Spatial Trends from Open Cluster Observations

open access: yesUniverse, 2022
Spectroscopic observations of stars belonging to open clusters, with well-determined ages and distances, are a unique tool for constraining stellar evolution, nucleosynthesis, mixing processes, and, ultimately, Galactic chemical evolution.
Laura Magrini   +8 more
doaj   +1 more source

BONNSAI: a Bayesian tool for comparing stars with stellar evolution models [PDF]

open access: yes, 2014
Powerful telescopes equipped with multi-fibre or integral field spectrographs combined with detailed models of stellar atmospheres and automated fitting techniques allow for the analysis of large number of stars.
Brott, Ines   +5 more
core   +3 more sources

The California-Kepler Survey. II. Precise Physical Properties of 2025 Kepler Planets and Their Host Stars [PDF]

open access: yes, 2017
We present stellar and planetary properties for 1305 Kepler Objects of Interest (KOIs) hosting 2025 planet candidates observed as part of the California-Kepler Survey.
Cargile, Phillip A.   +13 more
core   +3 more sources

An Independent Calibration of Stellar Ages: HST Observations of White Dwarfs at V=25 [PDF]

open access: yes, 1995
The white dwarf luminosity function of a stellar cluster will have a sharp truncation at a luminosity which is determined by the time since formation of the first white dwarfs in that cluster.
Gilmore, Gerard   +2 more
core   +3 more sources

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