Spectroscopy of Very Low Mass Stars and Brown Dwarfs in IC 2391: Lithium Depletion and Hα Emission

By D. B. Navascues, J. Stauffer, R. Jayawardhana. 2004

166 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/adedc7d87836b40413567b04635d9efd9c3eb86e

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS (2012, methodology): “An age of 50±5Myr was inferred by Barrado y Navascués et al. (2004) using lithium depletion and Hα emission.”
Painting a portrait of the Galactic disc with its stellar clusters (2020, methodology): “…spectroscopic measurements are available, the lithium depletion boundary method (LDB) can provide a better constraint than photometry (e.g. Barrado y Navascués et al. 2004; Jeffries & Oliveira 2005), but it can return older ages than CMD fitting (e.g. 21 Myr versus 7.5 Myr in Jeffries et al. 2017).”
BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc (2018, background): “References—(1) Mamajek 2016; (2) Bell et al. 2015; (3) Zuckerman et al. 2006; (4) Silaj & Landstreet 2014; (5) Gen- naro et al. 2012; (6) Murphy et al. 2013; (7) Brandt & Huang 2015; (8) Barrado y Navascués et al. 2004; (9) Dobbie et al. 2010; (10) Pecaut & Mamajek 2016; (11) Murphy & Lawson 2015; ”
THE HAWAII INFRARED PARALLAX PROGRAM. II. YOUNG ULTRACOOL FIELD DWARFS (2016, background): “…by Seifahrt et al. (2010) as candidates of the nearby moving groups studied by Montes et al. (2001): the Pleiades (1 object; 130±20 Myr [Barrado y Navascués et al. 2004]), Ursa Majoris (2 objects; ≈400–500 Myr [King et al. 2003; Jones et al. 2015]), and Hyades (4 objects; ≈600–800 Myr) moving…”
Time scales of Li evolution: A Homogeneous analysis of open clusters from ZAMS to late-MS (2005, methodology): “We mention in passing that Barrado y Navascués & Stauffer (1996) investigated a sample of Hyades binaries already observed by T93 finding that, whereas the general pattern is the same for double systems and single stars, binaries show slight over-abundances, that appear more conspicuous in tidally l”
A STELLAR CENSUS OF THE TUCANA–HOROLOGIUM MOVING GROUP (2014, result): “Barrado y Navascués et al. (2004) reported a boundary at Mbol = 10.24± 0.15 in IC 2391, as well as updating the results of Stauffer et al. (1998, 1999) for α Per (Mbol = 11.31 ± 0.15) and the Pleiades (Mbol = 12.14 ± 0.15).”
The Formation and Early Evolution of Low-Mass Stars and Brown Dwarfs (2012, background): “Examples of such populations include σ Ori (Béjar, Zapatero Osorio & Rebolo 1999), λOri (Barrado y Navascués et al. 2004), and Upper Sco (Slesnick, Carpenter & Hillenbrand 2006).”
The stellar and sub-stellar IMF of simple and composite populations (2011, background): “…classification of individual stars to place them on a theoretical isochrone of existing classical pre-main-sequence evolution theory to estimate masses (e.g. Meyer et al. 2000; Luhman 2004; Barrado y Navascués et al. 2004; Slesnick et al. 74 7 THE IMF OF LOW-MASS STARS (LMSS) 7.4 Star clusters 75”