J/ApJ/862/138   BANYAN. XIII. Nearby young assoc. with Gaia DR2   (Gagne+, 2018)

BANYAN. XIII. A first look at nearby young associations with Gaia Data Release 2. Gagne J., Faherty J.K. <Astrophys. J., 862, 138 (2018)> =2018ApJ...862..138G 2018ApJ...862..138G
ADC_Keywords: Stars, late-type; Proper motions; Radial velocities; Parallaxes, trigonometric; Spectral types; Associations, stellar Keywords: methods: data analysis; proper motions; stars: kinematics and dynamics Abstract: In this paper, we examine the nearest 100pc entries in Data Release 2 of Gaia to identify previously unrecognized candidate members in young associations. We analyze 695952 stars with the BANYAN Σ Bayesian classification software and discover 898 new high-likelihood candidate members that span a wide range of properties, from spectral types B9 to L2, including 104 comoving systems, 111 brown dwarfs, and 31 new bona fide members. Our sample is mostly composed of highly active M dwarfs and will be crucial in examining the low-mass end of the initial mass function of young associations. Our sample includes new candidate members near the Galactic plane where previous surveys suffered from a high rate of contamination. This paper represents the first step toward a full reassessment of young associations in the solar neighborhood with the second data release of the Gaia mission. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 71 20 Nearby young associations considered here table2.dat 135 898 New candidates identified in this work table3.dat 106 218 Co-moving systems identified in this work table5.dat 98 31 New bona fide members refs.dat 84 72 References -------------------------------------------------------------------------------- See also: III/10 : G5 and later stars in a North Galactic Pole region (Upgren 1962) III/190 : WEB Catalog of Radial Velocities (Duflot+ 1995) III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997) III/231 : The Tycho-2 Spectral Type Catalog (Wright+, 2003) II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012) II/359 : The VISTA Hemisphere Survey (VHS) catalog DR4.1 (McMahon+, 2013) III/279 : RAVE 5th data release (Kunder+, 2017) V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015) J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995) J/ApJS/101/117 : UBVRIJHKLMNQ photometry in Taurus-Auriga (Kenyon+ 1995) J/A+AS/123/329 : New weak-line T Tauri stars in Lupus (Krautter+ 1997) J/AJ/123/2828 : Spectroscopy of northern NLTT stars (Cruz+, 2002) J/AJ/123/3409 : SDSS M, L, and T dwarfs (Hawley+, 2002) J/AJ/126/2421 : 2MASS-Selected sample of ultracool dwarfs (Cruz+, 2003) J/AJ/126/2048 : NStars project: the Northern Sample. 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New members from Gaia-Tycho (Gagne+, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 A6 --- Assoc Name of the young association (1) 8- 12 F5.1 pc omega [25.4/130] Peak of distance distribution 14- 17 F4.1 pc e_omega [0.7/20] 1σ negative uncertainty 19- 22 F4.1 pc E_omega [0.8/30]? 1σ positive uncertainty 24- 28 F5.1 km/s nu [-12/39] Peak of radial velocity distribution 30- 33 F4.1 km/s e_nu [0.8/20] 1σ negative uncertainty 35- 38 F4.1 km/s E_nu [0.8/10]? 1σ positive uncertainty 40- 43 F4.1 pc Sspa [1.2/22.4] Characteristic spatial scale in XYZ space 45- 47 F3.1 km/s Skin [0.5/3.6] Characteristic kinematic scale in UVW space 49 A1 --- u_Age [~] Uncertainty flag on Age 50- 54 F5.1 Myr Age [1/750] Age (or lower range of Age) 55 A1 --- --- [-] 56 I1 Myr Age2 [2]? Upper range of Age 58- 62 F5.1 Myr e_Age [1.4/100]? Negative uncertainty 64- 67 F4.1 Myr E_Age [2/98]? Positive uncertainty 69- 71 I3 --- Ref [101/112] Reference (see refs.dat file) -------------------------------------------------------------------------------- Note (1): Full names of young associations as follows: 118Tau = 118 Tau association ABDMG = AB Doradus moving group BPMG = β Pictoris moving group CAR = Carina association CARN = Carina-Near moving group CBER = Coma Berenices cluster COL = Columba association EPSC = ε Chamaeleontis association HYA = the Hyades cluster LCC = Lower Centaurus Crux association OCT = Octans association PL8 = Platais 8 THA = the Tucana-Horologium association THOR = 32 Orionis association TWA = TW Hya UCL = Upper Centaurus Lupus association UMA = the core of the Ursa Major cluster USCO = Upper Scorpius association TAU = Taurus star-forming region XFOR = ξ1 For cluster -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- ID Source identifier (JHHMM+DDMM) 12 A1 --- f_SpT [p] p: estimated from the absolute Gaia G-band magnitude 13- 20 A8 --- SpT Spectral type 22- 27 A6 --- Assoc Association identifier (as in table 1) 32- 33 I2 h RAh [0/23] Hour of Right Ascension (J2000) (G1) 35- 36 I2 min RAm Minute of Right Ascension (J2000) 38- 43 F6.3 s RAs Second of Right Ascension (J2000) 45- 45 A1 --- DE- Sign of the Declination (J2000)(G1) 46- 47 I2 deg DEd Degree of Declination (J2000) (G1) 49- 50 I2 arcmin DEm Arcminute of Declination (J2000) 52- 56 F5.2 arcsec DEs Arcsecond of Declination (J2000) 58- 64 F7.2 mas/yr pmRA [-576/336] Proper motion along RA times cos(DE) 66- 69 F4.2 mas/yr e_pmRA [0.03/3.8] Uncertainty in pmRA 71- 77 F7.2 mas/yr pmDE [-452/448] Proper motion along DE 79- 82 F4.2 mas/yr e_pmDE [0.03/4.2] Uncertainty in pmDE 84- 89 F6.2 mas plx [10/113] Parallax 91- 94 F4.2 mas e_plx [0.02/3.4] Uncertainty in plx 96-100 F5.1 km/s RVel [-23/45]? Radial velocity 102-105 F4.1 km/s e_RVel [0.1/10]? Uncertainty in RVel 107-129 A23 --- Amb Identifiers of possible associations for ambiguous candidates (1) 131-132 I2 --- r_SpT [1/60]? Reference for SpT (see refs.dat file) 134-135 I2 --- r_RVel [1/53]? Reference for RVel (see refs.dat file) -------------------------------------------------------------------------------- Note (1): List of associations in ambiguous cases with their relative probabilities (%) between parentheses. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- Gaia Gaia DR2 identifier 21- 25 A5 --- Assoc Association ID as in Table 1 (1) 27- 31 F5.1 arcsec Sep [0.6/116]? Separation between component and host (2) 33- 34 I2 h RAh [0/23] Hour of Right Ascension (J2000) (G1) 36- 37 I2 min RAm Minute of Right Ascension (J2000) 39- 44 F6.3 s RAs Second of Right Ascension (J2000) 46 A1 --- DE- Sign of the Declination (J2000)(G1) 47- 48 I2 deg DEd Degree of Declination (J2000) (G1) 50- 51 I2 arcmin DEm Arcminute of Declination (J2000) 53- 57 F5.2 arcsec DEs Arcsecond of Declination (J2000) 59- 65 F7.2 mas/yr pmRA [-202/239] Proper motion along RA times cos(DE) 67- 70 F4.2 mas/yr e_pmRA [0.03/3.3] Uncertainty in pmRA 72- 78 F7.2 mas/yr pmDE [-152/103] Proper motion along DE 80- 83 F4.2 mas/yr e_pmDE [0.04/2] Uncertainty in pmDE 85- 89 F5.2 mas plx [6/50.5] Parallax 91- 94 F4.2 mas e_plx [0.02/2] Uncertainty in plx 96-100 F5.1 km/s RVel [-42/45.1]? Radial velocity 102-105 F4.1 km/s e_RVel [0.2/10.1]? Uncertainty in RVel 106 A1 --- f_RVel [*] Flag on RVel (3) -------------------------------------------------------------------------------- Note (1): All entries with an association identifier were recovered in this work as a candidate member of this group. Note (2): The host system is the first entry without a separation that precedes a given entry. Note (3): * = A kinematic radial velocity derived from BANYAN Sigma by assuming membership in a young association. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- f_Name Flag on Name (1) 3- 25 A23 --- Name Star name 27- 34 A8 --- SpT MK spectral type 35 A1 --- f_SpT [p] p: estimated from the absolute Gaia G-band magnitude 37- 41 A5 --- Assoc Association ID as in table 1 43- 44 I2 h RAh [0/23] Hour of Right Ascension (J2000) (G1) 46- 47 I2 min RAm Minute of Right Ascension (J2000) 49- 53 F5.2 s RAs Second of Right Ascension (J2000) 55 A1 --- DE- Sign of the Declination (J2000)(G1) 56- 57 I2 deg DEd Degree of Declination (J2000) (G1) 59- 60 I2 arcmin DEm Arcminute of Declination (J2000) 62- 65 F4.1 arcsec DEs Arcsecond of Declination (J2000) 67 A1 --- l_Age Limit flag on Age 68- 74 A7 Myr Age Age range 76- 98 A23 --- Comov Comoving star name -------------------------------------------------------------------------------- Note (1): Flag as follows: n = New bona fide members c = Comovers with known bona fide members -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Ref Reference code 5- 23 A19 --- BibCode Bibcode of the reference 25- 49 A25 --- Auth First author's name(s) 51- 84 A34 --- Comm Comment -------------------------------------------------------------------------------- Global notes: Note (G1): J2000 position at epoch 2015 from the Gaia DR2 catalog. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Malo et al. Paper I. 2013ApJ...762...88M 2013ApJ...762...88M Cat. J/ApJ/762/88 Gagne et al. Paper II. 2014ApJ...783..121G 2014ApJ...783..121G Cat. J/ApJ/783/121 Malo et al. Paper III. 2014ApJ...788...81M 2014ApJ...788...81M Cat. J/ApJ/788/81 Malo et al. Paper IV. 2014ApJ...792...37M 2014ApJ...792...37M Gagne et al. Paper V. 2015ApJ...798...73G 2015ApJ...798...73G Cat. J/ApJ/798/73 Artigau et al. Paper VI. 2015ApJ...806..254A 2015ApJ...806..254A Gagne et al. Paper VII. 2015ApJS..219...33G 2015ApJS..219...33G Cat. J/ApJS/219/33 Boucher et al. Paper VIII. 2016ApJ...832...50B 2016ApJ...832...50B Gagne et al. Paper IX. 2017ApJS..228...18G 2017ApJS..228...18G Desrochers et al. Paper X. 2018ApJ...852...55D 2018ApJ...852...55D Gagne et al. Paper XI. 2018ApJ...856...23G 2018ApJ...856...23G Cat. J/ApJ/856/23 Gagne et al. Paper XII. 2018ApJ...860...43G 2018ApJ...860...43G Cat. J/ApJ/860/43 Gagne et al. Paper XIII. 2018ApJ...862..138G 2018ApJ...862..138G This catalog
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 31-Jul-2019
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