J/MNRAS/503/3279   GALAH survey. Galactic disc with open clusters (Spina+, 2021)

The GALAH survey: tracing the Galactic disc with open clusters. Spina L., Ting Y.-S., De Silva G.M., Frankel N., Sharma S., Cantat-Gaudin T., Joyce M., Stello D., Karakas A.I., Asplund M.B., Nordlander T., Casagrande L., D'Orazi V., Casey A.R., Cottrell P., Tepper-Garcia T., Baratella M., Kos J., Cotar K., Bland-Hawthorn J., Buder S., Freeman K.C., Hayden M.R., Lewis G.F., Lin J., Lind K., Martell S.L., Schlesinger K.J., Simpson J.D., Zucker D.B., Zwitter T. <Mon. Not. R. Astron. Soc., 503, 3279-3296 (2021)> =2021MNRAS.503.3279S 2021MNRAS.503.3279S (SIMBAD/NED BibCode)
ADC_Keywords: Milky Way ; Clusters, open ; Abundances Keywords: stars: abundances - stars: kinematics and dynamics - Galaxy: abundances - Galaxy: disc - Galaxy: evolution - open clusters and associations: general Abstract: Open clusters are unique tracers of the history of our own Galaxy's disc. According to our membership analysis based on Gaia astrometry, out of the 226 potential clusters falling in the footprint of the GALactic Archaeology with HERMES (GALAH) survey or the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey, we find that 205 have secure members that were observed by at least one of the surveys. Furthermore, members of 134 clusters have high-quality spectroscopic data that we use to determine their chemical composition. We leverage this information to study the chemical distribution throughout the Galactic disc of 21 elements, from C to Eu. The radial metallicity gradient obtained from our analysis is -0.076±0.009dex/kpc, which is in agreement with previous works based on smaller samples. Furthermore, the gradient in the [Fe/H]-guiding radius (rguid) plane is -0.073±0.008dex/kpc. We show consistently that open clusters trace the distribution of chemical elements throughout the Galactic disc differently than field stars. In particular, at the given radius, open clusters show an age-metallicity relation that has less scatter than field stars. As such scatter is often interpreted as an effect of radial migration, we suggest that these differences are due to the physical selection effect imposed by our Galaxy: clusters that would have migrated significantly also had higher chances to get destroyed. Finally, our results reveal trends in the [X/Fe]-rguid-age space, which are important to understand production rates of different elements as a function of space and time. Description: In this study, we make use of three data sets: Gaia DR2 (Gaia Collaboration, 2018A&A...616A...1G 2018A&A...616A...1G, Cat. I/345), APOGEE DR16 (Ahumada et al., 2020ApJS..249....3A 2020ApJS..249....3A) and GALAH+ (Wittenmyer et al., 2018AJ....155...84W 2018AJ....155...84W; Sharma et al., 2018, Cat. J/MNRAS/473/2004, 2019MNRAS.490.5335S 2019MNRAS.490.5335S; Buder et al., 2020, arXiv:2011.02505). In this work, we used astrometric information from Gaia to identify the stellar members of the 226 open clusters that potentially fall in the footprints of the APOGEE or GALAH survey. Stellar coordinates and astrometric solutions from Gaia are used for cluster membership analysis. Radial velocities (RVs) provided by either Gaia, APOGEE, or GALAH. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 607 105684 Cluster membership probabilities analysis and cross-match with the GALAH and APOGEE data sets for 226 clusters table2.dat 452 205 Physical and kinematic properties of open clusters table3.dat 380 134 Chemical properties of open clusters -------------------------------------------------------------------------------- See also: I/345 : Gaia DR2 (Gaia Collaboration, 2018) III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020) J/A+A/640/A1 : Portrait Galactic disc (Cantat-Gaudin+, 2020) J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.7 deg RAdeg [0.0/360.0] Right Ascension (J2000) 13- 23 F11.7 deg DEdeg [-76.62/85.94] Declination (J2000) 25- 43 I19 --- GaiaDR2 Gaia DR2 source id 45- 59 I15 --- GALAH ? GALAH sobject id 61- 78 A18 --- APOGEE APOGEE ID 80- 92 A13 --- Cluster Cluster name 94- 97 F4.2 --- Pmem [0/1] Membership Probability (this work) 99-101 F3.1 --- PmemCG20 [0/1] Membership Probability (Cantat-Gaudin et al., 2020, Cat. J/A+A/640/A1) 103-109 F7.1 K Teff [4003/6997]? Effective temperature 111-116 F6.1 K e_Teff [65/208]? Error on Effective temperature 118-123 F6.3 [m/s2] logg [0.86/4.98]? Surface gravity 125-130 F6.3 [m/s2] e_logg [0.02/7.95]? Error on Surface gravity 132-137 F6.3 --- [Fe/H] [-1.0/0.44]? Metallicity [Fe/H] 139-144 F6.3 --- e_[Fe/H] [0/0.4]? Error on [Fe/H] 146-151 A6 --- r_param Origin for Stellar Parameters (apogee or galah) 153-158 F6.3 km/s vt [0.3/2.5]? Microturbolence velocity 160-167 F8.3 m/s RV [-987.82/845.37]? Radial Velocity 169-174 A6 --- r_RV Origin for Radial Velocity (apogee, gaia or galah) 176-181 F6.3 --- [C/Fe] [-0.67/1.21]? [C/Fe] abundance 183-188 F6.3 --- e_[C/Fe] [0/0.22]? Error on [C/Fe] 190-195 A6 --- r_[C/Fe] Origin for [C/Fe] (apogee or galah) 197-202 F6.3 --- [O/Fe] [-1.61/2.44]? [O/Fe] abundance 204-209 F6.3 --- e_[O/Fe] [0.0/0.29]? Error on [O/Fe] 211-216 A6 --- r_[O/Fe] Origin for [O/Fe] (apogee or galah) 218-223 F6.3 --- [Na/Fe] [-1.79/1.4]? [Na/Fe] abundance 225-230 F6.3 --- e_[Na/Fe] [0.02/0.3]? Error on [Na/Fe] 232-237 A6 --- r_[Na/Fe] Origin for [Na/Fe] (apogee or galah) 239-244 F6.3 --- [Mg/Fe] [-0.8/1.36]? [Mg/Fe] abundance 246-251 F6.3 --- e_[Mg/Fe] [0/0.33]? Error on [Mg/Fe] 253-258 A6 --- r_[Mg/Fe] Origin for [Mg/Fe] (apogee or galah) 260-265 F6.3 --- [Al/Fe] [-2.36/2.02]? [Al/Fe] abundance 267-272 F6.3 --- e_[Al/Fe] [0.01/0.19]? Error on [Al/Fe] 274-279 A6 --- r_[Al/Fe] Origin for [Al/Fe] (apogee or galah) 281-286 F6.3 --- [Si/Fe] [-0.63/1.4]? [Si/Fe] abundance 288-293 F6.3 --- e_[Si/Fe] [0/0.3]? Error on [Si/Fe] 295-300 A6 --- r_[Si/Fe] Origin for [Si/Fe] (apogee or galah) 302-307 F6.3 --- [Ca/Fe] [-1.2/1.52]? [Ca/Fe] abundance 309-314 F6.3 --- e_[Ca/Fe] [0/0.26]? Error on [Ca/Fe] 316-321 A6 --- r_[Ca/Fe] Origin for [Ca/Fe] (apogee or galah) 323-328 F6.3 --- [Ti/Fe] [-0.93/2.13]? [Ti/Fe] abundance 330-335 F6.3 --- e_[Ti/Fe] [0.01/0.5]? Error on [Ti/Fe] 337-342 A6 --- r_[Ti/Fe] Origin for [Ti/Fe] (apogee or galah) 344-349 F6.3 --- [V/Fe] [-1.06/1.87]? [V/Fe] abundance 351-356 F6.3 --- e_[V/Fe] [0.01/0.45]? Error on [V/Fe] 358-363 A6 --- r_[V/Fe] Origin for [V/Fe] (apogee or galah) 365-370 F6.3 --- [Cr/Fe] [-0.56/1.41]? [Cr/Fe] abundance 372-377 F6.3 --- e_[Cr/Fe] [0.02/0.24]? Error on [Cr/Fe] 379-383 A5 --- r_[Cr/Fe] Origin for [Cr/Fe] (apogee or galah) 385-390 F6.3 --- [Mn/Fe] [-1.31/1.73]? [Mn/Fe] abundance 392-397 F6.3 --- e_[Mn/Fe] [0/0.32]? Error on [Mn/Fe] 399-404 A6 --- r_[Mn/Fe] Origin for [Mn/Fe] (apogee or galah) 406-411 F6.3 --- [Co/Fe] [-1.85/2.82]? [Co/Fe] abundance 413-418 F6.3 --- e_[Co/Fe] [0.0/0.3]? Error on [Co/Fe] 420-425 A6 --- r_[Co/Fe] Origin for [Co/Fe] (apogee or galah) 427-432 F6.3 --- [Ni/Fe] [-0.91/1.48]? [Ni/Fe] abundance 434-439 F6.3 --- e_[Ni/Fe] [0.0/0.3]? Error on [Ni/Fe] 441-446 A6 --- r_[Ni/Fe] Origin for [Ni/Fe] (apogee or galah) 448-453 F6.3 --- [Cu/Fe] [-1.6/1.45]? [Cu/Fe] abundance 455-460 F6.3 --- e_[Cu/Fe] [0.01/0.3]? Error on [Cu/Fe] 462-467 A6 --- r_[Cu/Fe] Origin for [Cu/Fe] (apogee or galah) 469-474 F6.3 --- [Zn/Fe] [-1.07/1.47]? [Zn/Fe] abundance 476-481 F6.3 --- e_[Zn/Fe] [0.03/0.48]? Error on [Zn/Fe] 483-487 A5 --- r_[Zn/Fe] Origin for [Zn/Fe] (apogee or galah) 489-494 F6.3 --- [Y/Fe] [-1.24/1.78]? [Y/Fe] abundance 496-501 F6.3 --- e_[Y/Fe] [0.04/0.56]? Error on [Y/Fe] 503-507 A5 --- r_[Y/Fe] Origin for [Y/Fe] (apogee or galah) 509-514 F6.3 --- [Zr/Fe] [-0.44/2.3]? [Zr/Fe] abundance 516-521 F6.3 --- e_[Zr/Fe] [0/0.29]? Error on [Zr/Fe] 523-527 A5 --- r_[Zr/Fe] Origin for [Zr/Fe] (apogee or galah) 529-534 F6.3 --- [Ba/Fe] [-0.86/1.79]? [Ba/Fe] abundance 536-541 F6.3 --- e_[Ba/Fe] [0.03/0.3]? Error on [Ba/Fe] 543-547 A5 --- r_[Ba/Fe] Origin for [Ba/Fe] (apogee or galah) 549-554 F6.3 --- [La/Fe] [-0.33/2.46]? [La/Fe] abundance 556-561 F6.3 --- e_[La/Fe] [0/0.29]? Error on [La/Fe] 563-567 A5 --- r_[La/Fe] Origin for [La/Fe] (apogee or galah) 569-574 F6.3 --- [Nd/Fe] [-0.18/1.81]? [Nd/Fe] abundance 576-581 F6.3 --- e_[Nd/Fe] [0/0.29]? Error on [Nd/Fe] 583-587 A5 --- r_[Nd/Fe] Origin for [Nd/Fe] (apogee or galah) 589-594 F6.3 --- [Eu/Fe] [-0.34/1.72]? [Eu/Fe] abundance 596-601 F6.3 --- e_[Eu/Fe] [0/0.18]? Error on [Eu/Fe] 603-607 A5 --- r_[Eu/Fe] Origin for [Eu/Fe] (apogee or galah) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Cluster Cluster name 15- 18 F4.2 [yr] logAge [7.02/9.86] Age (log(Age/yr)) 20- 23 I4 --- Nmemb [12/2920] Number of members 25- 34 F10.6 deg RAdeg [1.09/359.77] Right Ascension (J2000) 36- 45 F10.6 deg s_RAdeg [0.01/142.35] Standard deviation on Right Ascension 47- 56 F10.6 deg DEdeg [-72.53/85.25] Declination (J2000) 58- 65 F8.6 deg s_DEdeg [0.01/5.18] Standard deviation on Declination 67- 72 F6.3 mas plx [0.0/20.94] Parallax 74- 78 F5.3 mas s_plx [0.02/2.59] Standard deviation on Parallax 80- 87 F8.3 mas/yr pmRA [-36.15/101.62] Proper motion along RA 89- 94 F6.3 mas/yr s_pmRA [0.05/25.36] Standard deviation on pmra 96-102 F7.3 mas/yr pmDE [-45.53/12.71] Proper motion along DE 104-109 F6.3 mas/yr s_pmDE [0.05/15.77] Standard deviation on pmdec 111-115 F5.3 kpc dist [0.04/8.17] Distance 117-121 F5.3 kpc s_dist [0.0/2.17] Standard deviation on Distance 123-129 F7.4 kpc XXYZ [5.11/15.86] Galactic X in cartesian coordinates XYZ 131-136 F6.4 kpc e_XXYZ [0.0/2.04] Error on Galactic X in cartesian coordinates XYZ 138-144 F7.4 kpc YXYZ [-6.61/4.2] Galactic Y in cartesian coordinates XYZ 146-151 F6.4 kpc e_YXYZ [0.0/1.84] Error on Galactic Y in cartesian coordinates XYZ 153-159 F7.4 kpc ZXYZ [-1.37/1.18] Galactic Z in cartesian coordinates XYZ 161-166 F6.4 kpc e_ZXYZ [0.0/0.57] Error on Galactic Z in cartesian coordinates XYZ 168-175 F8.3 km/s ULSR [-171.33/373.57] Cartesian U velocity in LSR 177-182 F6.3 km/s e_ULSR [0.01/51.68] Error on Cartesian U velocity in LSR 184-191 F8.3 km/s VLSR [-915.69/246.78] Cartesian V velocity in LSR 193-198 F6.3 km/s e_VLSR [0.11/39.09] Error on Cartesian V velocity in LSR 200-206 F7.3 km/s WLSR [-42.28/35.35] Cartesian W velocity in LSR 208-213 F6.3 km/s e_WLSR [0.31/11.0] Error on Cartesian W velocity in LSR 215-221 F7.4 kpc RRzphi [5.67/16.05] Galactic R in cylindrical coordinates Rzphi 223-228 F6.4 kpc e_RRzphi [0.0/2.11] Error on Galactic R in cylindrical coordinates Rzphi 230-236 F7.4 rad phiRzphi [-0.83/0.63] Galactic phi in cylindrical coordinates Rzphi 238-243 F6.4 rad e_phiRzphi [0.0/0.2] Error on Galactic phi in cylindrical coordinates Rzphi 245-251 F7.4 kpc zRzphi [-1.37/1.18] Galactic z in cylindrical coordinates Rzphi 253-258 F6.4 kpc e_zRzphi [0.0/0.57] Error on Galactic z in cylindrical coordinates Rzphi 260-267 F8.3 km/s vRRzphi [-585.17/60.85] Cylindrical vR velocity 269-274 F6.3 km/s e_vRRzphi [0.01/37.67] Error on Cylindrical vR velocity 276-283 F8.3 mas/s vphiRzphi [-507.58/501.21] Cylindrical vphi velocity 285-290 F6.3 mas/s e_vphiRzphi [0.12/38.87] Error on Cylindrical vphi velocity 292-298 F7.3 km/s vzRzphi [-34.79/42.42] Cylindrical vz velocity 300-305 F6.3 km/s e_vzRzphi [0.31/10.96] Error on Cylindrical vz velocity 307-319 F13.4 kpc.km/s JR [0.15/18727601.28] Radial Action 321-328 F8.4 kpc.km/s e_JR [0.0/179.17] Error on Radial Action 330-338 F9.3 kpc.km/s LZ [-5010.76/4024.65] Angular Momentum 340-346 F7.3 kpc.km/s e_LZ [1.02/472.19] Error on Angular Momentum 348-353 F6.3 kpc.km/s JZ [0.01/32.54] Vertical Action 355-360 F6.3 kpc.km/s e_JZ [0.0/19.38] Error on Vertical Action 362-367 F6.4 --- ecc [0.0/0.3]?=0 Orbit Eccentricity 369-374 F6.4 --- e_ecc [0.0/0.13]?=0 Error on Orbit Eccentricity 376-381 F6.3 kpc zmax [0.01/2.46]? Maximun height above the plane 383-387 F5.3 kpc e_zmax [0.0/1.06]?=0 Error on z max 389-396 F8.4 kpc Rperi [4.7/13.05]? Orbit Periastron 398-403 F6.4 kpc e_Rperi [0.0/2.41]?=0 Error on Orbit Periastron 405-412 F8.4 kpc Rap [5.83/20.12]? Orbit Apoastron 414-419 F6.4 kpc e_Rap [0.0/5.58]?=0 Error on Orbit Apoastron 421-430 F10.2 km2/s2 Energy [-68376.75/239389.47] Orbit Energy 432-439 F8.2 km2/s2 e_Energy [28.32/11371.35] Error on Orbit Energy 441-446 F6.3 kpc Rguid [5.2/24.93] Guiding radius 448-452 F5.3 kpc e_Rguid [0.0/2.37] Error on Guiding radius -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Cluster Cluster name 15- 20 F6.3 --- [Fe/H] [-0.63/0.34] [Fe/H] abundance 22- 26 F5.3 --- e_[Fe/H] [0.0/0.17] Error on [Fe/H] 28- 30 I3 --- o_[Fe/H] [1/168]?=0 Number of cluster members for [Fe/H] 32- 37 F6.3 --- [O/Fe] [-0.31/0.46]? [O/Fe] abundance 39- 44 F6.3 --- e_[O/Fe] [0.0/0.33]? Error on [O/Fe] 46- 47 I2 --- o_[O/Fe] [0/98]?=0 Number of cluster members for [O/Fe] 49- 54 F6.3 --- [Na/Fe] [-0.24/0.57]? [Na/Fe] abundance 56- 61 F6.3 --- e_[Na/Fe] [0.0/0.29]? Error on [Na/Fe] 63- 65 I3 --- o_[Na/Fe] [0/106]?=0 Number of cluster members for [Na/Fe] 67- 72 F6.3 --- [Mg/Fe] [-0.17/0.12]? [Mg/Fe] abundance 74- 79 F6.3 --- e_[Mg/Fe] [0.0/0.15]? Error on [Mg/Fe] 81- 83 I3 --- o_[Mg/Fe] [0/128]?=0 Number of cluster members for [Mg/Fe] 85- 90 F6.3 --- [Al/Fe] [-0.13/0.33]? [Al/Fe] abundance 92- 97 F6.3 --- e_[Al/Fe] [0.0/0.16]? Error on [Al/Fe] 99-101 I3 --- o_[Al/Fe] [0/129]?=0 Number of cluster members for [Al/Fe] 103-108 F6.3 --- [Si/Fe] [-0.11/0.19]? [Si/Fe] abundance 110-115 F6.3 --- e_[Si/Fe] [0.0/0.15]? Error on [Si/Fe] 117-119 I3 --- o_[Si/Fe] [0/129]?=0 Number of cluster members for [Si/Fe] 121-126 F6.3 --- [Ca/Fe] [0.0/0.28]? [Ca/Fe] abundance 128-133 F6.3 --- e_[Ca/Fe] [0.0/0.17]? Error on [Ca/Fe] 135-137 I3 --- o_[Ca/Fe] [0/126]?=0 Number of cluster members for [Ca/Fe] 139-144 F6.3 --- [Ti/Fe] [-0.14/0.49]? [Ti/Fe] abundance 146-151 F6.3 --- e_[Ti/Fe] [0.0/0.2]? Error on [Ti/Fe] 153-155 I3 --- o_[Ti/Fe] [0/113]?=0 Number of cluster members for [Ti/Fe] 157-162 F6.3 --- [V/Fe] [-0.15/0.65]? [V/Fe] abundance 164-169 F6.3 --- e_[V/Fe] [0.0/0.26]? Error on [V/Fe] 171-172 I2 --- o_[V/Fe] [0/65]?=0 Number of cluster members for [V/Fe] 174-179 F6.3 --- [Cr/Fe] [-0.13/0.15]? [Cr/Fe] abundance 181-186 F6.3 --- e_[Cr/Fe] [0.0/0.13]? Error on [Cr/Fe] 188-189 I2 --- o_[Cr/Fe] [0/96]?=0 Number of cluster members for [Cr/Fe] 191-196 F6.3 --- [Mn/Fe] [-0.16/0.19]? [Mn/Fe] abundance 198-203 F6.3 --- e_[Mn/Fe] [0.0/0.14]? Error on [Mn/Fe] 205-207 I3 --- o_[Mn/Fe] [0/123]?=0 Number of cluster members for [Mn/Fe] 209-214 F6.3 --- [Co/Fe] [-0.46/0.57]? [Co/Fe] abundance 216-221 F6.3 --- e_[Co/Fe] [0.0/0.44]? Error on [Co/Fe] 223-225 I3 --- o_[Co/Fe] [0/103]?=0 Number of cluster members for [Co/Fe] 227-232 F6.3 --- [Ni/Fe] [-0.24/0.3]? [Ni/Fe] abundance 234-239 F6.3 --- e_[Ni/Fe] [0.0/0.17]? Error on [Ni/Fe] 241-243 I3 --- o_[Ni/Fe] [0/127]?=0 Number of cluster members for [Ni/Fe] 245-250 F6.3 --- [Cu/Fe] [-0.27/0.27]? [Cu/Fe] abundance 252-257 F6.3 --- e_[Cu/Fe] [0.0/0.25]? Error on [Cu/Fe] 259-261 I3 --- o_[Cu/Fe] [0/122]?=0 Number of cluster members for [Cu/Fe] 263-268 F6.3 --- [Zn/Fe] [-0.25/0.29]? [Zn/Fe] abundance 270-275 F6.3 --- e_[Zn/Fe] [0.0/0.26]? Error on [Zn/Fe] 277-278 I2 --- o_[Zn/Fe] [0/97]?=0 Number of cluster members for [Zn/Fe] 280-285 F6.3 --- [Y/Fe] [-0.13/0.57]? [Y/Fe] abundance 287-292 F6.3 --- e_[Y/Fe] [0.03/0.37]? Error on [Y/Fe] 294-295 I2 --- o_[Y/Fe] [0/93]?=0 Number of cluster members for [Y/Fe] 297-302 F6.3 --- [Zr/Fe] [-0.05/0.31]? [Zr/Fe] abundance 304-309 F6.3 --- e_[Zr/Fe] [0.04/0.55]? Error on [Zr/Fe] 311-312 I2 --- o_[Zr/Fe] [0/33]?=0 Number of cluster members for [Zr/Fe] 314-319 F6.3 --- [Ba/Fe] [-0.08/0.81]? [Ba/Fe] abundance 321-326 F6.3 --- e_[Ba/Fe] [0.0/0.18]? Error on [Ba/Fe] 328-329 I2 --- o_[Ba/Fe] [0/98]?=0 Number of cluster members for [Ba/Fe] 331-336 F6.3 --- [La/Fe] [-0.23/0.75]? [La/Fe] abundance 338-343 F6.3 --- e_[La/Fe] [0.01/0.28]? Error on [La/Fe] 345-346 I2 --- o_[La/Fe] [0/51]?=0 Number of cluster members for [La/Fe] 348-353 F6.3 --- [Nd/Fe] [-0.02/0.93]? [Nd/Fe] abundance 355-360 F6.3 --- e_[Nd/Fe] [0.02/0.53]? Error on [Nd/Fe] 362-363 I2 --- o_[Nd/Fe] [0/28]?=0 Number of cluster members for [Nd/Fe] 365-370 F6.3 --- [Eu/Fe] [-0.23/0.6]? [Eu/Fe] abundance 372-377 F6.3 --- e_[Eu/Fe] [0.01/0.2]? Error on [Eu/Fe] 379-380 I2 --- o_[Eu/Fe] [0/18]?=0 Number of cluster members for [Eu/Fe] -------------------------------------------------------------------------------- Acknowledgements: Lorenzo Spina, spina.astro(at)gmail.com
(End) Patricia Vannier [CDS] 01-Jun-2021
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