The AB Doradus Moving Group

By B. Zuckerman, Inseok Song, M. Bessell. 2004

178 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f427bc7b233596080cea5a66078920b476c3d4fa

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In Astronomy and Astrophysics

1. Eric Mamajek
2. Michael C. Liu
3. B. Bowler
4. A. Burgasser
5. K. Luhman
6. T. Dupuy
7. Kelle Cruz
8. E. Shkolnik

Citations in the corpus

• The Hipparcos–Gaia Catalog of Accelerations (2018, background): “…have enabled the discovery and mapping of Galactic streams (Koppelman et al. 2018), of stellar moving groups with ever-expanding membership lists (Zuckerman et al. 2001, 2004; Malo et al. 2013; Gagné & Faherty 2018), measurements of the proper motions of globular clusters and dwarf galaxies…”
• The Nearest Young Moving Groups (2006, methodology): “Very recently, Zuckerman et al. (2004) have identified a large group of stars with the same space motion than the well-known young K-dwarf AB Dor (d = 15 pc), a quadruple system (Close et al. 2005; Guirado et al. 2006) made up of three late-type stars — AB Dor A (HD 36705), AB Dor Ba and AB Dor Bb…”
• BAYESIAN ANALYSIS TO IDENTIFY NEW STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS (2012, methodology): “An age of∼ 50 Myr is deduced by a color-magnitude diagram (CMD) (MV vs V − K; see figure 1 of Zuckerman et al. 2004).”
• Search for associations containing young stars (SACY). I. Sample and searching method (2006, background): “…et al. (2001b); the β Pic Association (BPA) (d ∼ 35 pc; age ∼ 15 Myr; Barrado y Navascués 1998; Zuckerman et al. 2001a); the AB Dor Association (d ∼ 20 pc; age ∼ 50 Myr; Zuckerman et al. 2004; Torres et al. 2003, - calling it as AnA); and finally two less well defined associations, the Argus…”
• BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc (2018, background): “…et al. 1989; Kastner et al. 1997), β Pictoris (βPMG; Zuckerman et al. 2001a), Tucana-Horologium (THA; Torres et al. 2000; Zuckerman et al. 2001b), Carina (CAR; Torres et al. 2008), Columba (COL; Torres et al. 2008), Argus (ARG; Makarov & Urban 2000) and AB Doradus (ABDMG; Zuckerman et al. 2004).”
• THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS (2013, background): “Since then, >20 TW Hya members have been identified (see Webb et al. 1999; Sterzik et al. 1999; Jayawardhana et al. 1999; Zuckerman et al. 2001c, 2004; Gizis 2002; Song et al. 2002, 2003; Kastner et al. 2008; Scholz et al. 2005; Mamajek 2005; Looper et al. 2007; Torres et al. 2008; Fernández et…”
• 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…”
• WIDE COMPANIONS TO HIPPARCOS STARS WITHIN 67 pc OF THE SUN (2012, background): “At larger scales of∼1 pc we also encounter co-moving remnants of nearby clusters and associations (e.g. Zuckerman et al. 2001, 2004).”
• A companion to AB Pic at the planet/brown dwarf boundary (2005, background): “…al. 2000, Zuckerman & Webb 2000) and TW Hydrae (Kastner et al. 1997) associations, as well as theβ Pictoris (Zuckerman et al. 2001) and AB Doradus (Zuckerman et al. 2004) co-moving groups, to explore the circumstellarnvironment within semimajor axes between tens and hundreds of AU with detection…”
• PLANETS AROUND LOW-MASS STARS (PALMS). IV. THE OUTER ARCHITECTURE OF M DWARF PLANETARY SYSTEMS (2014, unknown): “…(2008), (11) Torres et al. (2000) (12) Zuckerman et al. (2001), (13) Kraus et al. (2014), (14) Torres et al. (2003), (15) Silva et al. (2013), (16) Zuckerman et al. (2004), (17) Ortega et al. (2007), (18) Luhman et al. (2005), (19) Barenfeld et al. (2013), (20) Barrado y Navascués (1998), (21)…”
• BANYAN. II. VERY LOW MASS AND SUBSTELLAR CANDIDATE MEMBERS TO NEARBY, YOUNG KINEMATIC GROUPS WITH PREVIOUSLY KNOWN SIGNS OF YOUTH (2013, unknown): “5 for the two components, and estimate their age to be around 100 Myr because of their low surface gravity.”
• HAZMAT. I. THE EVOLUTION OF FAR-UV AND NEAR-UV EMISSION FROM EARLY M STARS (2014, unknown): “…(2006), 12: Zuckerman et al. (2001), 13: Looper et al. (2010), 14: Shkolnik et al. (2012), 15: Kraus et al. (2014), 16: Montes et al. (2001), 17: Zuckerman et al. (2004), 18: Malo et al. (2013), 19: López-Santiago et al. (2006), 20: Bowler et al. (2012), 21: Ammler-von Eiff & Guenther (2009),…”
• CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS (2015, background): “0 V, pEW(Hα) = –3.4+0.5 −0.3 Å, V577 Per B), a confirmed member of the∼70 Ma-old AB Doradus moving group (Zuckerman et al. 2004; da Silva et al. 2009; Schlieder et al. 2012a).”
• BANYAN. VII. A NEW POPULATION OF YOUNG SUBSTELLAR CANDIDATE MEMBERS OF NEARBY MOVING GROUPS FROM THE BASS SURVEY (2015, background): “…& Webb 2000; Zuckerman et al. 2001b; Kraus et al. 2014b), Carina (CAR; 20–40 Myr; Torres et al. 2008), Columba (COL; 20–40 Myr; Torres et al. 2008), Argus (ARG; 30–50 Myr; Makarov & Urban 2000) and AB Doradus (ABDMG; 110– 130 Myr; Zuckerman et al. 2004; Luhman et al. 2005; Barenfeld et al. 2013).”