2018A&A...615A..51M


Query : 2018A&A...615A..51M

2018A&A...615A..51M - Astronomy and Astrophysics, volume 615A51-51 (2018/7-1)

Dynamical ages of the young local associations with Gaia.

MIRET-ROIG N., ANTOJA T., ROMERO-GOMEZ M. and FIGUERAS F.

Abstract (from CDS):


Context. The young local associations (YLAs) constitute an excellent sample for the study of a variety of astrophysical topics, especially the star formation process in low-density environments. Data from the Gaia mission allows us to undertake studies of the YLAs with unprecedented accuracy.
Aims. We determine the dynamical age and place of birth of a set of associations in a uniform and dynamically consistent manner. There are nine YLAs in our sample ε Chamaeleontis, TW Hydrae, β Pictoris, Octans, Tucana-Horologium, Columba, Carina, Argus, and AB Doradus.
Methods. We designed a method for deriving the dynamical age of the YLAs based on the orbital integration. The method involves a strategy to account for the effect of observational errors. We tested the method using mock YLAs. Finally, we applied it to our set of nine YLAs with astrometry from the first Gaia data release and complementary on-ground radial velocities from the literature.
Results. Our orbital analysis yields a first estimate of the dynamical age of 33–0+9Myr, 1313–0+7Myr, and 55–0+23Myr for ε Chamaeleontis, β Pictoris, and Tucana-Horologium, respectively. For four other associations (Octans, Columba, Carina, and Argus), we provide a lower limit for the dynamical age. Our rigorous error treatment indicates that TW Hydrae and AB Doradus deserve further study.
Conclusions. The dynamical ages that we obtain are compatible spectroscopic and isochrone fitting ages obtained elsewhere. From the orbital analysis, we suggest a scenario for these YLAs where there were two episodes of star formation: one ∼40Myr ago in the first quadrant that gave birth to ε Chamaeleontis, TW Hydrae, and β Pictoris, and another 5-15Myr ago close to the Sun that formed Tucana-Horologium, Columba, and Carina. Future Gaia data will provide the necessary accuracy to improve the present results, especially for the controversial age determinations, and additional evidence for the proposed scenario once a complete census of YLAs and better membership can be obtained.

Abstract Copyright: © ESO 2018

Journal keyword(s): Galaxy: kinematics and dynamics - solar neighborhood - open clusters and associations: general - stars: kinematics and dynamics - stars: formation

Errata: erratum vol. 618, art. C7 (2018)

Simbad objects: 31

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Number of rows : 31
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME THA MGr 00 00 -62.0           ~ 540 0
2 NAME Lindblad Ring DNe 02 16 45 +64 21.5           ~ 44 0
3 HD 14082B BY* 02 17 24.7369490496 +28 44 30.411007188   8.33 7.74     G3 123 0
4 HD 14082 BY* 02 17 25.2869702592 +28 44 42.145069812   7.545 7.031 8.04   F2 137 0
5 Cl Melotte 25 OpC 04 30 27.4 +16 46 43           ~ 3309 0
6 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
7 NAME 32 Ori group OpC 05 27 11 +06 16.0           ~ 84 0
8 NAME Columba Association As* 06 04 19.4 -22 20 40           ~ 337 0
9 NAME AB Dor Moving Group MGr 06 38 53.4 -42 50 04           ~ 540 0
10 Cl Mamajek 1 OpC 08 42 32.9 -78 57 47           ~ 392 0
11 NAME Car Arm PoG 10 00 -60.0           ~ 471 1
12 HD 298936 PM* 10 13 14.7724609728 -52 30 54.001503468   10.81 9.763   8.687 K3Ve 69 0
13 V* BX Ant TT* 10 18 28.6987521312 -31 50 02.830052544   13.39 11.454 11.382 9.325 M0Ve 130 0
14 V* TW Hya TT* 11 01 51.9053285064 -34 42 17.033218380   11.94 10.50 10.626 9.18 K6Ve 2144 1
15 NAME TW Hya Association As* 11 01.9 -34 42           ~ 1018 0
16 CD-33 7795 TT* 11 31 55.2608963280 -34 36 27.203892120   12.97 11.524 11.150 9.150 M2Ve 205 0
17 HD 102458 Or* 11 47 24.5438206248 -49 53 03.018484572   9.70 9.07   8.40 G4V 102 0
18 CD-36 7429 ** 11 48 24.22320 -37 28 49.1537           ~ 98 0
19 NAME eps Cha Association OpC 11 59 51 -78 12.4           ~ 188 0
20 V* V1249 Cen TT* 12 15 30.7203201048 -39 48 42.606684144   13.09 11.160 10.919 9.50 M0.5 139 0
21 NAME beta Pic Moving Group MGr 14 30 -42.0           ~ 894 0
22 NAME Upper Sco-Cen As* 16 15 -24.2           ~ 1497 1
23 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
24 HD 155555 RS* 17 17 25.5053342232 -66 57 03.732141636 7.795 7.499 6.723   6.39 G5V+K1V 292 1
25 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
26 HD 164249 PM* 18 03 03.4097283792 -51 38 56.432149872   7.438 7.007 7.90   F6V 142 0
27 HD 181327 PM* 19 22 58.9437222504 -54 32 16.975668624   7.50 7.04   6.49 F6V 331 0
28 NAME Octans Association As* ~ ~           ~ 101 0
29 NAME Galactic Bar reg ~ ~           ~ 1458 0
30 NAME Carina Association As* ~ ~           ~ 188 1
31 NAME Argus Association As* ~ ~           ~ 266 0

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