Works matching IS 17439213 AND DT 2008 AND VI 4 AND IP S258
Results: 46
Stellar age dating with thorium, uranium and lead.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 449, doi. 10.1017/S1743921309032104
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Stellar ages from asteroseismology: a few examples.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 443, doi. 10.1017/S1743921309032098
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The Sun as a fundamental calibrator of stellar evolution.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 431, doi. 10.1017/S1743921309032086
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Stellar ages from asteroseismology.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 419, doi. 10.1017/S1743921309032074
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The promise of Gaia and how it will influence stellar ages.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 409, doi. 10.1017/S1743921309032062
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The Sun in time: age, rotation, and magnetic activity of the Sun and solar-type stars and effects on hosted planets.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 395, doi. 10.1017/S1743921309032050
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Isochrones for late-type stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 383, doi. 10.1017/S1743921309032049
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How accurately can we age-date solar-type dwarfs using activity/rotation diagnostics?
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 375, doi. 10.1017/S1743921309032037
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The rotational evolution of low-mass stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 363, doi. 10.1017/S1743921309032025
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Stellar ages from stellar rotation.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 357, doi. 10.1017/S1743921309032013
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Gyrochronology and its usage for main sequence field star ages.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 345, doi. 10.1017/S1743921309032001
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Confronting substellar theoretical models with stellar ages.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 337, doi. 10.1017/S1743921309031998
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Using magnetic activity and Galactic dynamics to constrain the ages of M dwarfs.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 327, doi. 10.1017/S1743921309031986
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Brown dwarfs as Galactic chronometers.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 317, doi. 10.1017/S1743921309031974
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Towards a precise white dwarf cooling age of a globular cluster.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 315, doi. 10.1017/S1743921309031962
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Stellar chronology with white dwarfs in wide binaries.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 307, doi. 10.1017/S1743921309031950
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White dwarfs as astrophysical probes.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 299, doi. 10.1017/S1743921309031949
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White dwarf cosmochronology: Techniques and uncertainties.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 287, doi. 10.1017/S1743921309031937
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The star clusters of the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 275, doi. 10.1017/S1743921309031925
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The ages of Galactic globular clusters in the context of self-enrichment.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 265, doi. 10.1017/S1743921309031913
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Multiple population theory: The extreme helium population problem.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 253, doi. 10.1017/S1743921309031901
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Recovering the ages and metallicities of stars of a complex stellar population system.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 245, doi. 10.1017/S1743921309031895
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Observations of multiple populations in star clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 233, doi. 10.1017/S1743921309031883
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Relative and absolute ages of Galactic globular clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 221, doi. 10.1017/S1743921309031871
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The ages of stars: The horizontal branch.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 209, doi. 10.1017/S174392130903186X
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Homogeneous photometry of globular clusters—a progress report.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 197, doi. 10.1017/S1743921309031858
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A new method to estimate the ages of globular clusters: the case of NGC 3201.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 189, doi. 10.1017/S1743921309031846
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Models for Pop I stars: implications for age determinations.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 177, doi. 10.1017/S1743921309031834
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Globular cluster ages from main sequence fitting and detached, eclipsing binaries: The case of 47 Tuc.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 171, doi. 10.1017/S1743921309031822
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Eclipsing binary stars as tests of stellar evolutionary models and stellar ages.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 161, doi. 10.1017/S1743921309031810
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The Bologna Open Cluster Chemical Evolution project: a large, homogeneous sample of Galactic open clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 153, doi. 10.1017/S1743921309031809
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Observational problems in determining the ages of open clusters.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 141, doi. 10.1017/S1743921309031792
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On the use of lithium to derive the ages of stars like our Sun.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 133, doi. 10.1017/S1743921309031780
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Using ages and kinematic traceback: the origin of young local associations.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 123, doi. 10.1017/S1743921309031779
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Circumstellar disk evolution: Constraining theories of planet formation.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 111, doi. 10.1017/S1743921309031767
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New methods for determining the ages of PMS stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 103, doi. 10.1017/S1743921309031755
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Age spreads in star forming regions?
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 95, doi. 10.1017/S1743921309031743
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Age-related observations of low mass pre-main and young main sequence stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 81, doi. 10.1017/S1743921309031731
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The ACS LCID project: Variable stars as tracers of population gradients.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 73, doi. 10.1017/S174392130903172X
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Star formation histories of resolved galaxies.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 61, doi. 10.1017/S1743921309031718
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The star formation history of the Magellanic Clouds.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 51, doi. 10.1017/S1743921309031706
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The timescales of chemical enrichment in the Galaxy.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 39, doi. 10.1017/S174392130903169X
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Signatures of heating processes in the Galactic thin disk.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 31, doi. 10.1017/S1743921309031688
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The age of the Galaxy's thick disk.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 23, doi. 10.1017/S1743921309031676
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The star-formation history of the Milky Way Galaxy.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 11, doi. 10.1017/S1743921309031664
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Some problems in studying the ages of stars.
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- Proceedings of the International Astronomical Union, 2008, v. 4, n. S258, p. 1, doi. 10.1017/S1743921309031652
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- Article