Young Stars Near the Sun

By B. Zuckerman, Inseok Song. 2004

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View Paper: https://www.semanticscholar.org/paper/6124cc4100cfeb05d3f6b377cf6351bd3a4685b6

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In Astronomy and Astrophysics

Citations in the corpus

Giant Planet Companion to 2MASSW J1207334-393254 (2005, background): “For example, according to measurements of isotopes of hafnium-tungsten in meteorites and in the mantle, it is deduced that Earth’s core likely formed in less than 30 million years (see Zuckerman & Song 2004).”
THE TUCANA/HOROLOGIUM, COLUMBA, AB DORADUS, AND ARGUS ASSOCIATIONS: NEW MEMBERS AND DUSTY DEBRIS DISKS (2011, methodology): “Characteristic mean UVW for Tuc/Hor stars are given in Zuckerman & Song (2004) as -11, -21, 0 km s−1, and in Torres et al. (2008) as -9.9±1.5, -20.9±0.8, -1.4±0.9 km s−1.”
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS (2013, methodology): “We adopted AAVSO Photometric All-Sky Survey (APASS) Data Release 6 (Henden et al. 2012) BV and SACY (Torres et al. 2006) BV IC photometry where available.”
Characterization of Dusty Debris Disks: The IRAS and Hipparcos Catalogs (2006, methodology): “Estimation of the age of a star that belongs to a known kinematic stellar group (Zuckerman & Song 2004b) is relatively straightforward.”
Discovery of a Very Young Field L Dwarf, 2MASS J01415823–4633574 (2005, background): “(See review by Zuckerman & Song 2004.)”
THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS (2013, background): “Over 50 stars have been identified to date in the AB Dor moving group (Zuckerman & Song 2004; Torres et al. 2008; Fernández et al. 2008; da Silva (A color version of this figure is available in the online journal.) et al. 2009; Schlieder et al. 2010, 2012; Zuckerman et al. 2011; Shkolnik et al.…”
BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc (2018, methodology): “These include the convergent point tool (e.g., Mamajek 2005; Torres et al. 2006; Rodriguez et al. 2011), various goodnessof-fit metrics (e.g. Kraus et al. 2014; Bowler et al. 2017; Shkolnik et al. 2017), and the “good box” method (Zuckerman & Song 2004).”
BANYAN. VII. A NEW POPULATION OF YOUNG SUBSTELLAR CANDIDATE MEMBERS OF NEARBY MOVING GROUPS FROM THE BASS SURVEY (2015, background): “If this system is younger than∼ 200 Myr, the individual mass of each component would be well below the deuterium burning limit, which would make it a remarkable benchmark system to understand the properties of planetary-mass objects.”
The Gemini Deep Planet Survey (2007, methodology): “For other stars that have lithium and/or X-ray measurements, ages were estimated from a comparison of the Li I 6708 Å equivalent width and/or the ratio of the X-ray to bolometric luminosity with Figures 3 and/or 4 of Zuckerman & Song (2004b) respectively.”
A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood (2015, methodology): “6 Tuc-Hor GJ 3054 (HIP 3556), HD 12894, HD 200798, and BS Ind (HD 202947) are all designated members of Tuc-Hor by Zuckerman & Song (2004), however Malo et al. (2013) demonstrated that if their radial velocities are included as priors, their respective probabilities of belonging to Tuc-Hor…”
The Ages of Stars (2007, background): “However, there are a number of groups of very young stars near to the Sun (see Zuckerman & Song (2004)) that have members with Hipparcos astrometry.”
Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics (2008, methodology): “…Pleiades B4 moving group (Asiain et al. 1999; Famaey et al. 2007) has been demonstrated, and (3) the range of acceptable velocities for membership in the AB Dor group seems rather large for a coeval group (Zuckerman & Song 2004) compared to OB associations and clusters (e.g. Briceño et al. 2007).”
The Formation and Early Evolution of Low-Mass Stars and Brown Dwarfs (2012, background): “The nearest samples of young stars to the Sun (d < 100 pc) are found in small moving groups and associations (Zuckerman et al. 2011, Zuckerman & Song 2004).”
A Moving Cluster Distance to the Exoplanet 2M1207b in the TW Hydrae Association (2005, background): “I add to TWA numbers 1 through 25 (Zuckerman & Song 2004) the three, new, low-mass candidate members 2M1207 and 2MASSW J1139511-315921 from Gizis (2002), and SSSPM J1102-3431 from Scholz et al. (2005).”
DISCOVERIES FROM A NEAR-INFRARED PROPER MOTION SURVEY USING MULTI-EPOCH TWO MICRON ALL-SKY SURVEY DATA (2010, background): “This distance estimate places it further away than any of the young associations studied by Zuckerman & Song (2004) or Torres et al. (2008).”
THE HAWAII INFRARED PARALLAX PROGRAM. II. YOUNG ULTRACOOL FIELD DWARFS (2016, background): “Several field L dwarfs from Seifahrt et al. (2010) were included in our sample, as they were re- ported to be candidate members of older (&100 Myr) moving groups, namely the Hyades, Pleaides, Ursa Major streams (e.g. Montes et al. 2001; Zuckerman & Song 2004).”
A giant planet candidate near a young brown dwarf - Direct VLT/NACO observations using IR wavefront sensing (2004, methodology): “A K-band brightness difference between young (∼10 Myr) and old late M-type stars can be estimated and 2.5 mag is obtained by extrapolating trends of young and old mid-M stars in a V −K vs. MK diagram of Song et al. (2003) and Zuckerman & Song (2004).”
The AB Doradus Moving Group (2004, methodology): “A similar range of spectral types is seen in previously discovered nearby moving groups with ages in the range 8–30 Myr (Table 2; Zuckerman & Song 2004).”
A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group (2013, methodology): “The mean Galactic space motion of the BPMG (U, V, W) = (−11, −16,−9 kms−1) and convergent point (05h 19m 48s,−60d 13m 12s, Zuckerman & Song 2004), leads to a predicted RV for group members as a function of their sky position.”
BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS (2012, methodology): “We propose that HIP 17782 AB be assigned asbona fide memberof COL. HIP 2484 AbB: This star was proposed by Zuckerman & Song (2004) to be a member of THA.”