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相关论文: Inferring the Age of the Universe with Globular Cl…

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This is the third article in a series aimed at computing accurate and precise ages of galactic globular clusters from their full color-magnitude diagram in order to estimate the age of the Universe and in turn constrain the cosmological…

宇宙学与河外天体物理 · 物理学 2025-03-26 David Valcin , Raul Jimenez , Uroš Seljak , Licia Verde

We revisit the determination of the age of the Universe from galactic globular clusters, extending previous analyses by explicitly accounting for the presence of multiple stellar populations within each cluster. Using high--quality…

星系天体物理 · 物理学 2026-03-06 David Valcin , Raul Jimenez , Carmela Lardo , Uroš Seljak , Licia Verde

Globular clusters are the oldest objects in the Galaxy whose age may be accurately determined. As such globular cluster ages provide the best estimate for the age of the universe. The age of a globular cluster is determined by a comparison…

天体物理学 · 物理学 2009-10-28 Brian Chaboyer

The main sequence turnoff luminosity is the best stellar `clock' which can be used to determine the absolute ages of globular clusters. This is due to the fact that it is generally assumed that the luminosity and lifetimes of main sequence…

天体物理学 · 物理学 2009-10-22 Brian Chaboyer

We report the results of a detailed numerical study designed to estimate both the absolute age and the uncertainty in age (with confidence limits) of the oldest globular clusters. Such an estimate is essential if a comparison with the…

天体物理学 · 物理学 2009-10-28 Brian Chaboyer , Peter J. Kernan , Lawrence M. Krauss , Pierre Demarque

The dominant systematic uncertainty in the age determination of galactic globular clusters is the depth of the convection envelope of the stars. This parameter is partially degenerate with metallicity which is in turn degenerate with age.…

星系天体物理 · 物理学 2022-01-24 David Valcin , Raul Jimenez , Licia Verde , Jose Luis Bernal , Benjamin D. Wandelt

I review here recent developments which have affected our understanding of both the absolute age of globular clusters and the uncertainties in this age estimate, and comment on the implications for cosmological models. This present estimate…

天体物理学 · 物理学 2014-10-13 Lawrence M. Krauss

We review five independent techniques which are used to set the distance scale to globular clusters, including subdwarf main sequence fitting utilizing the recent Hipparcos parallax catalogue. These data together all indicate that globular…

天体物理学 · 物理学 2009-10-30 Brian Chaboyer , P. Demarque , Peter J. Kernan , Lawrence M. Krauss

Globular clusters are the oldest conglomerates of stars in our Galaxy and can be useful laboratories to test theories from stellar evolution to cosmology. In this paper, we present a new method to estimate the absolute age of a globular…

太阳与恒星天体物理 · 物理学 2017-02-02 Ilaria Caiazzo , Jeremy S. Heyl , Harvey Richer , Jason Kalirai

In the past 40 years a considerable effort has been focused in determining the age of the Universe at zero redshift using several stellar clocks. In this review I will describe the best theoretical methods to determine the age of the oldest…

天体物理学 · 物理学 2007-05-23 R. Jimenez

We present accurate relative ages for a sample of 55 Galactic globular clusters. The ages have been obtained by measuring the difference between the horizontal branch and the turnoff in two, internally photometrically homogeneous databases.…

天体物理学 · 物理学 2009-07-28 F. De Angeli , G. Piotto , S. Cassisi , G. Busso , A. Recio-Blanco , M. Salaris , A. Aparicio , A. Rosenberg

Estimating the age of the Universe is an old problem. Rapid progress in observational cosmology in recent years has led to more accurate values of the fundamental parameters. The current most popular model is a flat Universe, with about 30%…

天体物理学 · 物理学 2007-05-23 Oleg Y. Gnedin , Ofer Lahav , Martin J. Rees

Ages of extragalactic globular clusters can provide valuable insights into the formation and evolution of galaxies. In this contribution the photometric methods of age dating old globular cluster systems are summarised. The spectroscopic…

天体物理学 · 物理学 2009-11-07 Thomas H. Puzia

There are three independent techniques for determining the age of the universe: via cosmochronology of long-lived radioactive nuclei, via stellar modelling and population synthesis of the oldest stellar populations, and via the precision…

天体物理学 · 物理学 2009-11-06 I. Ferreras , A. Melchiorri , J. Silk

We present a new method to compute stellar ages in Globular Clusters (GC) that is ten times more precise than the traditional isochrone fitting procedure. The method relies on accurate stellar evolutionary tracks and on photometry for GCs…

天体物理学 · 物理学 2016-08-30 Raul Jimenez , Paolo Padoan

A minimum age of the universe can be estimated directly by determining the age of the oldest objects in the our Galaxy. These objects are the metal-poor stars in the halo of the Milky Way. Recent work on nucleochronology finds that the…

天体物理学 · 物理学 2009-10-30 Brian Chaboyer

We determine the age of 1,104 early-type galaxies in eight rich clusters ($z = 0.0046$ to $0.175$) using a new continuum color technique. We find that galaxies in clusters divide into two populations, an old population with a mean age…

天体物理学 · 物理学 2009-11-13 K. Rakos , J. Schombert , A. Odell

Globular clusters (GCs) provide statistically significant coeval populations of stars spanning various evolutionary stages, allowing robust constraints on stellar evolution model parameters and ages. We analyze eight old Milky Way GCs with…

星系天体物理 · 物理学 2025-05-07 Jiaqi , Ying , Brian Chaboyer , Michael Boylan-Kolchin , Daniel Weisz , Rowan Goebel-Bain

We establish a framework for determing absolute ages of Galactic globular clusters and then use these ages to investigate the age-metallicity and age-Galactocentric distance relations for the 36 clusters with the most reliable age data. The…

The age of three of the oldest clusters -- M15, M68, M92 -- has been redetermined. We use the latest EOS and opacity data available for calculating both isochrones and zero age horizontal branches and employ the brightness difference…

天体物理学 · 物理学 2009-10-28 M. Salaris , S. Degl'Innocenti , A. Weiss
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