New Members of the TW Hydrae Association, β Pictoris Moving Group, and Tucana/Horologium Association

By Inseok Song, B. Zuckerman, M. Bessell. 2003

160 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1cd398169b8fa616c1bc64dd8c02197c4141218b

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

1. Eric Mamajek
2. Michael C. Liu
3. B. Bowler
4. K. Luhman
5. A. Burgasser
6. T. Dupuy
7. M. Pecaut
8. C. Bell

Citations in the corpus

• The AB Doradus Moving Group (2004, unknown): “Details of our observations and results can and will be found in Song et al. (2003) and I. Song et al. (2004, in preparation).”
• Nearby Debris Disk Systems with High Fractional Luminosity Reconsidered (2006, background): “…25457 (50–100 Myr from moving group, Zuckerman & Song 2004b; 4000þ1200 2100 Myr from isochrones, Nordström et al. 2004), HD 164249 (12þ8 4 Myr, Song et al. 2003; 2200 þ1200 1800 Myr, Nordström et al. 2004), and HD 181327 (12þ8 4 Myr, Song et al. 2003; 1300þ1000 1300 Myr, Nordström et al. 2004).”
• BANYAN. II. VERY LOW MASS AND SUBSTELLAR CANDIDATE MEMBERS TO NEARBY, YOUNG KINEMATIC GROUPS WITH PREVIOUSLY KNOWN SIGNS OF YOUTH (2013, background): “NYAs represent interesting test benches for planetary formation theories, since 10 and 30 Myr respectively correspond to the formation timescales of giant and terrestrial planets (Song et al. 2003).”
• A companion to AB Pic at the planet/brown dwarf boundary (2005, background): “In March 2003, we observed the young star AB Pic (HIP 30034, K2V, V=9.16,d = 47.3+1.8 −1.7 pc), identified by Song et al. (2003) as a member of the large Tucana-Horologiumasso- Send offprint requests to: Gaël Chauvin e-mail:gchauvin@eso.org ⋆ Based on ESO observing programs 70.”
• HAZMAT. I. THE EVOLUTION OF FAR-UV AND NEAR-UV EMISSION FROM EARLY M STARS (2014, unknown): “…(2004), 4: Sterzik et al. (1999), 5: Gregorio-Hetem et al. (1992), 6: Torres et al. (2006), 7: Webb et al. (1999), 8: Shkolnik et al. (2011), 9: Song et al. (2003), 10: Reid (2003), 11: Jayawardhana et al. (2006), 12: Zuckerman et al. (2001), 13: Looper et al. (2010), 14: Shkolnik et al.…”
• Toward Planetesimals in the Disk around TW Hydrae: 3.5 Centimeter Dust Emission (2005, background): “The TW Hydrae association, which contains more than 20 stellar systems with ages estimated to be 5–10 Myr, is the nearest known site of recent star formation activity (Song et al. 2003).”
• THE TUCANA/HOROLOGIUM, COLUMBA, AB DORADUS, AND ARGUS ASSOCIATIONS: NEW MEMBERS AND DUSTY DEBRIS DISKS (2011, methodology): “As in our previous papers on these and other young, nearby, moving groups (e.g., Song et al 2003, Zuckerman et al 2004, Zuckerman et al 2001a and 2001b), we rely on a combination of techniques – including Galactic space motions UVW, location on color-magnitude diagrams, lithium abundance, and X-ray…”
• BANYAN. VII. A NEW POPULATION OF YOUNG SUBSTELLAR CANDIDATE MEMBERS OF NEARBY MOVING GROUPS FROM THE BASS SURVEY (2015, methodology): “This is reminiscent of 2MASS J12474428– 3816464, TWA 29 and TWA 31, which are young and seem to be located between TWA and SCC in terms of distance (Song et al. 2003; Schneider et al. 2012; Gagné et al. 2014a; Paper V).”
• Young Stars Near the Sun (2004, methodology): “Isochrones from solarmetallicity evolutionary models from four research groups (see Song et al. 2003) are plotted at 10 and 100 Myr.”
• The star formation history and accretion-disc fraction among the K-type members of the Scorpius–Centaurus OB association (2016, methodology): “Finally, we mention that the adopted kinematic expansion age of the β Pictoris moving group (BPMG) of 12 Myr, estimated by Song et al. (2003), has been re-evaluated by Mamajek & Bell (2014).”
• Imaging Extrasolar Giant Planets (2016, background): “Initial discoveries include two substellar companions: 2MASS J01225093–2439505 B, an L-type member of AB Dor at the planet/brown dwarf boundary with an unusually red spectrum (Bowler et al. 2013; Hinkley et al. 2015a), and 2MASS J02155892– 0929121 C (Bowler et al. 2015c), a brown dwarf in a close qu”
• A lithium depletion boundary age of 21 Myr for the Beta Pictoris moving group (2013, background): “Some estimates of kinematic ages, based on the traceback of candidate members to their smallest volume, also yield 10-12 Myr with very small formaluncertainties (Ortega et al. 2002, 2004; Song et al. 2003).”
• THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS (2013, background): “Over 60 members of the β Pic moving group have been identified to date (Song et al. 2003; Zuckerman & Song 2004; Torres et al. 2006, 2008; Fernández et al. 2008; da Silva et al. 2009; Lépine & Simon 2009; Rice et al. 2010; Schlieder et al. 2010; Kiss et al. 2011; Schlieder et al. (A color version…”
• On the age of the β Pictoris moving group (2014, methodology): “To infer a systematic expansion age of 11− 12 Myr for the BPMG, one would probably have to choose and omit particular objects (as did Song et al. 2003), however this would either negate the reliability of determining a global expansion rate for the whole group, or force one to significantly cut…”
• Giant Planet Companion to 2MASSW J1207334-393254 (2005, background): “This might be possible as TWA is possibly related to the sub-region Lower Centaurus-Crux of the recent massive star forming region Sco-Cen (Mamajek & Fiegelson 2001; Mamajek et al. 2002; Song et al. 2003).”
• Search for associations containing young stars (SACY). I. Sample and searching method (2006, methodology): “Song et al. (2003) also considered it as an outlier.”
• BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS (2012, methodology): “Following the advent of the 2MASS PSC catalog (Cutri et al. 2003), Song et al. (2003) used an opticalinfrared color-magnitude diagram to better discriminate between K and M dwarfs.”