Time scales of Li evolution: A Homogeneous analysis of open clusters from ZAMS to late-MS

By P. Sestito, S. Randich. 2005

195 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/1d2a2badb45034db123caa6da6dde5bf2a619b7b

How researchers see this paper

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In Astronomy and Astrophysics

1. Nuno C. Santos
2. S. Udry
3. J. Southworth
4. M. Mayor
5. C. Conroy
6. F. Pepe
7. C. Lovis
8. F. Bouchy

In Instrumentation

1. J. Southworth
2. Nuno C. Santos
3. S. Udry
4. C. Conroy
5. Benjamin D. Johnson
6. M. Mayor
7. F. Pepe
8. C. Lovis

Citations in the corpus

• WASP-19b: THE SHORTEST PERIOD TRANSITING EXOPLANET YET DISCOVERED (2010, background): “However, the nondetection of Li i in WASP-19 again gives only a weak constraint on the age suggesting the star is older than the Hyades (0.6 Myr; Sestito & Randich 2005).”
• The Ages of Stars (2007, background): “Sestito & Randich (2005) summarize and analyze the available Li data for OC stars.”
• Lithium depletion in solar-like stars: no planet connection (2010, methodology): “Data are from the compilation by Sestito & Randich (2005) as shown in Table 2 with updated data for M67 by Pasquini et al. (2008).”
• MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS (2016, background): “The purple square and circle are surface lithium abundance for the present-day Sun (Asplund et al. 2009) and the typical surface lithium abundance for nearby solar-metallicity, young clusters (e.g., Jeffries & Oliveira 2005; Sestito & Randich 2005; Juarez et al. 2014).”
• DIRECT IMAGING OF A COLD JOVIAN EXOPLANET IN ORBIT AROUND THE SUN-LIKE STAR GJ 504 (2013, background): “Extensive observations of well-dated open clusters (Sestito & Randich 2005) enable a lithium age estimate for GJ 504.”
• Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius (2009, unknown): “This nondetection points to an older age than the 0.6 Gyr of the Hyades (Sestito & Randich 2005). light curve (Fig.1), but also in the broad photospheric Caii H & K absorption lines (Fig.”
• The HARPS search for southern extra-solar planets IX. Exoplanets orbiting HD 100777, HD 190647, and HD 221287 (2007, background): “Studies of the lithium abundances of open cluster main sequence stars have shown that log n(Li) remains constant and equals ' 3 for Teff = 6300 K stars older than a few million years (see for example Sestito & Randich 2005).”