J/MNRAS/509/122               COMBS III                           (Lucey+, 2022)

The COMBS Survey. III. The chemodynamical origins of metal-poor bulge stars. Lucey M., Hawkins K., Ness M., Nelson T., Debattista V., Luna A., Bensby T., Freeman K.C., Kobayashi C. <Mon. Not. R. Astron. Soc. 509, 122-144 (2022)> =2022MNRAS.509..122L 2022MNRAS.509..122L (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Stars, population II ; Abundances ; Radial velocities ; Optical Keywords: stars: abundances - stars: Population II - Galaxy: bulge - Galaxy: evolution Abstract: The characteristics of the stellar populations in the Galactic bulge inform and constrain the Milky Way's formation and evolution. The metal-poor population is particularly important in light of cosmological simulations, which predict that some of the oldest stars in the Galaxy now reside in its centre. The metal-poor bulge appears to consist of multiple stellar populations that require dynamical analyses to disentangle. In this work, we undertake a detailed chemodynamical study of the metal-poor stars in the inner Galaxy. Using R ∼ 20 000 VLT/GIRAFFE spectra of 319 metal-poor (-2.55dex≤[Fe/H]≤0.83dex, with mean [Fe/H]=-0.84dex) stars, we perform stellar parameter analysis and report 12 elemental abundances (C, Na, Mg, Al, Si, Ca, Sc, Ti, Cr, Mn, Zn, Ba, and Ce) with precisions of ∼0.10 dex. Based on kinematic and spatial properties, we categorize the stars into four groups, associated with the following Galactic structures: the inner bulge, the outer bulge, the halo, and the disc. We find evidence that the inner and outer bulge population is more chemically complex (i.e. higher chemical dimensionality and less correlated abundances) than the halo population. This result suggests that the older bulge population was enriched by a larger diversity of nucleosynthetic events. We also find one inner bulge star with a [Ca/Mg] ratio consistent with theoretical pair-instability supernova yields and two stars that have chemistry consistent with globular cluster stars. Description: Based on observations collected at the European Southern Observator y under ESO programme: 089.B-069. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 1341 319 Chemodynamical properties of target stars (full table A1) -------------------------------------------------------------------------------- See also: J/MNRAS/488/2283 : COMBS survey. Galactic Bulge metal-poor stars (Lucey+, 2019) J/MNRAS/501/5981 : COMBS Survey. Metal-poor bulge stars (Lucey+, 2021) Byte-by-byte Description of file: table.* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Object Star identification number (object) 10- 14 F5.3 --- prob Probability that a star stays confined to the bulge (prob) 16- 24 F9.6 kpc peri Pericenter (peri) 26- 33 F8.6 kpc e_peri Lower value of peri interval (peri_lo) 35- 44 F10.6 kpc E_peri Upper value of peri interval (peri_hi) 46- 56 F11.6 kpc api Apocenter (api) 58- 66 F9.6 kpc e_api Lower value of api interval (api_lo) 68- 78 F11.6 kpc E_api Upper value of api interval (api_hi) 80- 88 F9.7 --- e Eccentricity (e) 90- 98 F9.7 --- e_e Lower value of e interval(e_lo) 100- 108 F9.7 --- E_e Upper value of e interval(e_hi) 110- 118 F9.6 pc zmax Maximun height above the plane (zmax) 120- 128 F9.6 pc e_zmax Lower value of zmax interval(zmax_lo) 130- 140 F11.6 pc E_zmax Upper value of zmax interval (zmax_hi) 142- 150 F9.3 kpc.km/s Lz Z component of Angular Momentum (Lz) 152- 157 F6.3 kpc.km/s e_Lz Lower value of Lz interval (Lz_lo) 159- 165 F7.3 kpc.km/s E_Lz Upper value of Lz interval (Lz_hi) 167- 175 F9.5 deg RAdeg Right ascension (ICRS) (RA) 177- 186 F10.6 deg DEdeg Declination (ICRS) (DEC) 188- 196 F9.6 mag Gmag G magnitude (G) 198- 205 F8.3 km/s RV Radial velocity (RV) 207- 214 F8.3 km/s e_RV Radial velocity error (e_RV) 216- 223 F8.3 km/s s_RV Radial velocity scatter (s_RV) 225- 226 I2 --- N6 Number of HR06 observations (N_6) 228 I1 --- N21 Number of HR21 observations (N_21) 230- 237 F8.4 --- SNR6 Signal-to-noise ratio of HR06 (SNR_6) 239- 246 F8.4 --- SNR21 Signal-to-noise ratio of HR21 (SNR_21) 248- 256 F9.5 deg GLON Galactic longitude (l) 258- 266 F9.5 deg GLAT Galactic latitude (b) 268- 273 F6.3 --- [Mg/H] ?=- Abundance [Mg/H] (Mg) 275- 279 F5.3 --- e_[Mg/H] ?=- Error on abundance [Mg/H] (Mg_err) 281- 286 F6.3 --- [Ti/H] ?=- Abundance [Ti/H] (Ti) 288- 292 F5.3 --- e_[Ti/H] ?=- Error on abundance [Ti/H] (Ti_err) 294- 299 F6.3 --- [Cr/H] ?=- Abundance [Cr/H] (Cr) 301- 305 F5.3 --- e_[Cr/H] ?=- Error on abundance [Cr/H] (Cr_err) 307- 312 F6.3 --- [Mn/H] ?=- Abundance [Mn/H] (Mn) 314- 318 F5.3 --- e_[Mn/H] ?=- Error on abundance [Mn/H] (Mn_err) 320- 325 F6.3 --- [Fe/H] ?=- Abundance [Fe/H] (Fe) 327- 331 F5.3 --- e_[Fe/H] ?=- Error on abundance [Fe/H] (Fe_err) 333- 338 F6.3 --- [Zn/H] ?=- Abundance [Zn/H] (Zn) 340- 344 F5.3 --- e_[Zn/H] ?=- Error on abundance [Zn/H] (Zn_err) 346- 351 F6.3 --- [Ba/H] ?=- Abundance [Ba/H] (Ba) 353- 357 F5.3 --- e_[Ba/H] ?=- Error on abundance [Ba/H] (Ba_err) 359- 364 F6.3 --- [Ce/H] ?=- Abundance [Ce/H] (Ce) 366- 370 F5.3 --- e_[Ce/H] ?=- Error on abundance [Ce/H] (Ce_err) 372- 377 F6.3 --- [Sc/H] ?=- Abundance [Sc/H] (Sc) 379- 383 F5.3 --- e_[Sc/H] ?=- Error on abundance [Sc/H] (Sc_err) 385- 390 F6.3 --- [Si/H] ?=- Abundance [Si/H] (Si) 392- 396 F5.3 --- e_[Si/H] ?=- Error on abundance [Si/H] (Si_err) 398- 403 F6.3 --- Mg4702.991 ?=- Abundance [Mg/H] from line at 4702.991 angstroms (Mg_4702.991) 405- 408 A4 --- e_Mg4702.991 ?=- Error on [Mg/H] abundance from line at 4702.991 angstroms (Mg4702.991err) 410- 415 F6.3 --- Mg8806.76 ?=- Abundance [Mg/H] from line at 8806.76 angstroms (Mg_8806.76) 417- 420 A4 --- e_Mg8806.76 ?=- Error on [Mg/H] abundance from line at 8806.76 angstroms (Mg8806.76err) 422- 427 F6.3 --- Ti4548.76 ?=- Abundance [Ti/H] from line at 4548.76 angstroms (Ti_4548.76) 429- 432 A4 --- e_Ti4548.76 ?=- Error on [Ti/H] abundance from line at 4548.76 angstroms (Ti4548.76err) ( 434- 439 F6.3 --- Ti4555.48 ?=- Abundance [Ti/H] from line at 4555.48 angstroms(Ti_4555.48) 441- 444 A4 --- e_Ti4555.48 ?=- Error on [Ti/H] abundance from line at 4555.48 angstroms (Ti4555.48err) 446- 451 F6.3 --- Cr4558.59 ?=- Abundance [Cr/H] from line at 4558.59 angstroms(Cr_4558.59) 453- 456 A4 --- e_Cr4558.59 ?=- Error on [Cr/H] abundance from line at 4558.59 angstroms (Cr4558.59err) 458- 463 F6.3 --- Cr4588.14 ?=- Abundance [Cr/H] from line at 4588.14 angstroms(Cr_4588.14) 465- 468 A4 --- e_Cr4588.14 ?=- Error on [Cr/H] abundance from line at 4588.14 angstroms (Cr4588.14err) 470- 475 F6.3 --- Cr4646.15 ?=- Abundance [Cr/H] from line at 4646.15 angstroms (Cr_4646.15) 477- 480 A4 --- e_Cr4646.15 ?=- Error on [Cr/H] abundance from line at 4646.15 angstroms (Cr4646.15err) 482- 487 F6.3 --- Cr4545.95 ?=- Abundance [Cr/H] from line at 4545.95 angstroms(Cr_4545.95) 489- 492 A4 --- e_Cr4545.95 ?=- Error on [Cr/H] abundance from line at 4545.95 angstroms (Cr4545.95err) 494- 499 F6.3 --- Cr4651.28 ?=- Abundance [Cr/H] from line at 4651.28 angstroms(Cr_4651.28) 501- 504 A4 --- e_Cr4651.28 ?=- Error on [Cr/H] abundance from line at 4651.28 angstroms (Cr4651.28err) 506- 511 F6.3 --- Cr4591.99 ?=- Abundance [Cr/H] from line at 4591.99 angstroms(Cr_4591.99) 513- 516 A4 --- e_Cr4591.99 ?=- Error on [Cr/H] abundance from line at 4591.99 angstroms (Cr4591.99err) 518- 523 F6.3 --- Mn4709.71 ?=- Abundance [Mn/H] from line at 4709.71 angstroms (Mn_4709.71) 525- 528 A4 --- e_Mn4709.71 ?=- Error on [Mn/H] abundance from line at 4709.71 angstroms (Mn4709.71err) 530- 535 F6.3 --- Fe8688.62 ?=- Abundance [Mg/H] from line at 4702.991 angstroms (Fe_8688.62) 537- 540 A4 --- e_Fe8688.62 ?=- Error on [Mg/H] abundance from line at 4702.991 angstroms (Fe8688.62err) 542- 547 F6.3 --- Fe8824.22 ?=- Abundance [Fe/H] from line at 8824.22 angstroms(Fe_8824.22) 549- 552 A4 --- e_Fe8824.22 ?=- Error on [Fe/H] abundance from line at 8824.22 angstroms (Fe8824.22err) 554- 559 F6.3 --- Fe4576.34 ?=- Abundance [Fe/H] from line at 4576.34 angstroms(Fe_4576.34) 561- 564 A4 --- e_Fe4576.34 ?=- Error on [Fe/H] abundance from line at 4576.34 angstroms (Fe4576.34err) 566- 571 F6.3 --- Fe4666.76 ?=- Abundance [Fe/H] from line at 4666.76 angstroms(Fe_4666.76) 573- 576 A4 --- e_Fe4666.76 ?=- Error on [Fe/H] abundance from line at 4666.76 angstroms (Fe4666.76err) 578- 583 F6.3 --- Fe4731.45 ?=- Abundance [Fe/H] from line at 4731.45 angstroms(Fe_4731.45) 585- 588 A4 --- e_Fe4731.45 ?=- Error on [Fe/H] abundance from line at 4731.45 angstroms (Fe4731.45err) 590- 595 F6.3 --- Zn4680.134 ?=- Abundance [Zn/H] from line at 4680.134 angstroms(Zn_4680.134) 597- 600 A4 --- e_Zn4680.134 ?=- Error on [Zn/H] abundance from line at 4680.134 angstroms (Zn4680.134err) 602- 607 F6.3 --- Zn4722.159 ?=- Abundance [Zn/H] from line at 4722.159 angstroms(Zn_4722.159) 609- 612 A4 --- e_Zn4722.159 ?=- Error on Zn/H] abundance from line at 4722.159 angstroms (Zn4722.159err) 614- 619 F6.3 --- Ba4554.03 ?=- Abundance [Ba/H] from line at 4554.03 angstroms(Ba_4554.03) 621- 624 A4 --- e_Ba4554.03 ?=- Error on [Ba/H] abundance from line at 4554.03 angstroms(Ba4554.03err) 626- 631 F6.3 --- Ce4628.16 ?=- Abundance [Ce/H] from line at 4628.16 angstroms(Ce_4628.16) 633- 636 A4 --- e_Ce4628.16 ?=- Error on [Ce/H] abundance from line at 4628.16 angstroms (Ce4628.16err) 638- 643 F6.3 --- Sc4670.42 ?=- Abundance [Sc/H] from line at 4670.42 angstroms(Sc_4670.42) 645- 648 A4 --- e_Sc4670.42 ?=- Error on [Sc/H] abundance from line at 4670.42 angstroms (Sc4670.42err) 650- 655 F6.3 --- Mg8717.83 ?=- Abundance [Mg/H] from line at 8717.83 angstroms (Mg_8717.83) 657- 660 A4 --- e_Mg8717.83 ?=- Error on [Mg/H] abundance from line at 8717.83 angstroms (Mg8717.83err) 662- 667 F6.3 --- Mg8923.57 ?=- Abundance [Mg/H] from line at 8923.57 angstroms (Mg_8923.57) 669- 672 A4 --- e_Mg8923.57 ?=- Error on [Mg/H] abundance from line at 8923.57 angstroms (Mg8923.57err) 674- 679 F6.3 --- Ti8682.98 ?=- Abundance [Ti/H] from line at 8682.98 angstroms (Ti_8682.98) 681- 684 A4 --- e_Ti8682.98 ?=- Error on [Ti/H] abundance from line at 8682.98 angstroms (Ti8682.98err) 686- 691 F6.3 --- Fe4602.94 ?=- Abundance [Fe/H] from line at 4602.94 angstroms (Fe_4602.94) 693- 696 A4 --- e_Fe4602.94 ?=- Error on [Fe/H] abundance from line at 4602.94 angstroms(Fe4602.94err) 698- 703 F6.3 --- Ce4562.36 ?=- Abundance [Ce/H] from line at 4562.36angstroms(Ce_4562.36) 705- 708 A4 --- e_Ce4562.36 ?=- Error on [Ce/H] abundance from line at 4562.36angstroms(Ce4562.36err) 710- 715 F6.3 --- Si8648.465 ?=- Abundance [Si/H] from line at 8648.465 angstroms (Si_8648.465) 717- 720 A4 --- e_Si8648.465 ?=- Error on [Si/H] abundance from line at 8648.465 angstroms (Si8648.465err) 722- 727 F6.3 --- Si8728.01 ?=- Abundance [Si/H] from line at 8728.01 angstroms (Si_8728.01) 729- 732 A4 --- e_Si8728.01 ?=- Error on [Si/H] abundance from line at 8728.01 angstroms (Si8728.01err) 734- 739 F6.3 --- Ti8734.71 ?=- Abundance [Ti/H] from line at 8734.71 angstroms (Ti_8734.71) 741- 744 A4 --- e_Ti8734.71 ?=- Error on [Ti/H] abundance from line at 8734.71 angstroms (Ti8734.71err) 746- 751 F6.3 --- Ti8692.329 ?=- Abundance [Ti/H] from line at 8692.329angstroms (Ti_8692.329) 753- 756 A4 --- e_Ti8692.329 ?=- Error on [Ti/H] abundance from line at 8692.329angstroms(Ti8692.329err) 758- 763 F6.3 --- Fe4602.01 ?=- Abundance [Fe/H] from line at 4602.01 angstroms (Fe_4602.01) 765- 768 A4 --- e_Fe4602.01 ?=- Error on [Fe/H] abundance from line at 4602.01 angstroms(Fe4602.01err) 770- 775 F6.3 --- Fe4602.95 ?=- Abundance [Fe/H] from line at 4602.95 angstroms (Fe_4602.95) 777- 780 A4 --- e_Fe4602.95 ?=- Error on [Fe/H] abundance from line at 4602.95 angstroms(Fe4602.95err) 782- 787 F6.3 --- [Ca/H] ?=- Abundance [Ca/H] (Ca) 789- 793 F5.3 --- e_[Ca/H] ?=- Error on abundance [Ca/H] (Ca_err) 795- 800 F6.3 --- Ca8912.07 ?=- Abundance [Ca/H] from line at 8912.07 angstroms (Ca_8912.07) 802- 805 A4 --- e_Ca8912.07 ?=- Error on [Ca/H] abundance from line at 8912.07 angstroms(Ca8912.07err) 807- 812 F6.3 --- Ca8927.36 ?=- Abundance [Ca/H] from line at 8927.36 angstroms (Ca_8927.36) 814- 817 A4 --- e_Ca8927.36 ?=- Error on [Ca/H] abundance from line at 8927.36 angstroms(Ca8927.36err) 819- 824 F6.3 --- Ca4578.55 ?=- Abundance [Ca/H] from line at 4578.55 angstroms(Ca_4578.55) 826- 829 A4 --- e_Ca4578.55 ?=- Error on [Ca/H] abundance from line at 4578.55 angstroms(Ca4578.55err) 831- 836 F6.3 --- Ca4586.04 ?=- Abundance [Ca/H] from line at 4586.04 angstroms(Ca_4586.04) 838- 841 A4 --- e_Ca4586.04 ?=- Error on [Ca/H] abundance from line at 4586.04 angstroms(Ca4586.04err) 843- 848 F6.3 --- Ca4685.27 ?=- Abundance [Ca/H] from line at 4685.27 angstroms (Ca_4685.27) 850- 853 A4 --- e_Ca4685.27 ?=- Error on [Ca/H] abundance from line at 4685.27 angstroms(Ca4685.27err) 855- 860 F6.3 --- [Na/H] ?=- Abundance [Na/H] (Na) 862- 866 F5.3 --- e_[Na/H] ?=- Error on abundance [Na/H] (Na_err) 868- 873 F6.3 --- [Al/H] ?=- Abundance [Al/H] (Al) 875- 879 F5.3 --- e_[Al/H] ?=- Error on abundance [Al/H] (Al_err) 881- 886 F6.3 --- Na4668.572 ?=- Abundance [Na/H] from line at 4668.572 angstroms(Na_4668.572) 888- 891 A4 --- e_Na4668.572 ?=- Error on [Na/H] abundance from line at 4668.572 angstroms (Na4668.572err) 893- 898 F6.3 --- Na4751.82 ?=- Abundance [Na/H] from line at 4751.82 angstroms(Na_4751.82) 900- 903 A4 --- e_Na4751.82 ?=- Error on [Na/H] abundance from line at 4751.82 angstroms(Na4751.82err) 905- 910 F6.3 --- Al8772.865 ?=- Abundance [Al/H] from line at 8772.865 angstroms (Al_8772.865) 912- 915 A4 --- e_Al8772.865 ?=- Error on [Al/H] abundance from line at 8772.865 angstroms (Al8772.865err) 917- 922 F6.3 --- Al8773.896 ?=- Abundance [Al/H] from line at 8773.896 angstroms (Al_8773.896) 924- 927 A4 --- e_Al8773.896 ?=- Error on [Al/H] abundance from line at 8773.896 angstroms (Al8773.896err) 929- 934 F6.3 --- Al8841.28 ?=- Abundance [Al/H] from line at 8841.28 angstroms (Al_8841.28) 936- 939 A4 --- e_Al8841.28 ?=- Error on [Al/H] abundance from line at 8841.28 angstroms (Al8841.28err) 941- 946 F6.3 --- Al8828.91 ?=- Abundance [Al/H] from line at 8828.91 angstroms (Al_8828.91) 948- 951 A4 --- e_Al8828.91 ?=- Error on [Al/H] abundance from line at 8828.91 angstroms (Al8828.91err) 953- 958 F6.3 --- [C/H] ?=- Abundance [C/H] (C) 960- 964 F5.3 --- e_[C/H] ?=- Error on abundance [C/H] (C_err) 966- 971 F6.3 --- C8727.0 ?=- Abundance [C/H] from line at 8727.0 angstroms (C_8727.0) 973- 976 A4 --- e_C8727.0 ?=- Error on [C/H] abundance from line at 8727.0 angstroms (C8727.0err) 978- 982 F5.3 --- s_[C/H] ?=- Scatter on abundance [C/H] (C_serr) 984- 988 F5.3 --- s_[Na/H] ?=- Scatter on abundance [Na/H] (Na_serr) 990- 994 F5.3 --- s_[Mg/H] ?=- Scatter on abundance [Mg/H] (Mg_serr) 996-1000 F5.3 --- s_[Al/H] ?=- Scatter on abundance [Al/H] (Al_serr) 1002-1006 F5.3 --- s_[Ca/H] ?=- Scatter on abundance [Ca/H] (Ca_serr) 1008-1012 F5.3 --- s_[Ti/H] ?=- Scatter on abundance [Ti/H] (Ti_serr) 1014-1018 F5.3 --- s_[Cr/H] ?=- Scatter on abundance [Cr/H] (Cr_serr) 1020-1024 F5.3 --- s_[Mn/H] ?=- Scatter on abundance [Mn/H] (Mn_serr) 1026-1030 F5.3 --- s_[Fe/H] ?=- Scatter on abundance [Fe/H] (Fe_serr) 1032-1036 F5.3 --- s_[Zn/H] ?=- Scatter on abundance [Zn/H] (Zn_serr) 1038-1042 F5.3 --- s_[Ba/H] ?=- Scatter on abundance [Ba/H] (Ba_serr) 1044-1048 F5.3 --- s_[Ce/H] ?=- Scatter on abundance [Ce/H] (Ce_serr) 1050-1054 F5.3 --- s_[Sc/H] ?=- Scatter on abundance [Sc/H] (Sc_serr) 1056-1060 F5.3 --- s_[Si/H] ?=- Scatter on abundance [Si/H] (Si_serr) 1062-1067 F6.3 --- s_[C/H]c []?=- Corrected abundance [C/H] (C_corr) 1069-1076 F8.3 km/s Uvel U velocity (U) 1078-1085 F8.3 km/s e_Uvel [] Lower value of U interval (U_lo) 1087-1094 F8.3 km/s E_Uvel [] Upper value of U interval (U_hi) 1096-1104 F9.3 km/s Vvel V velocity (V) 1106-1114 F9.3 km/s e_Vvel [] Lower value of V interval(V_lo) 1116-1123 F8.3 km/s E_Vvel [] Upper value of V interval(V_hi) 1125-1132 F8.3 km/s Wvel W velocity (W) 1134-1142 F9.3 km/s e_Wvel [] Lower value of W interval (W_lo) 1144-1151 F8.3 km/s E_Wvel [] Upper value of W interval(W_hi) 1153-1160 F8.5 pc Xpos X position (X) 1162-1169 F8.5 pc e_Xpos [] Lower value of X interval (X_lo) 1171-1179 F9.5 pc E_Xpos [] Upper value of X interval(X_hi) 1181-1188 F8.5 pc Ypos Y position (Y) 1190-1197 F8.5 pc e_Ypos [] Lower value of Y interval(Y_lo) 1199-1206 F8.5 pc E_Ypos [] Upper value of Y interval(Y_hi) 1208-1215 F8.5 pc Zpos Z position (Z) 1217-1225 F9.5 pc e_Zpos [] Lower value of Z interval(Z_lo) 1227-1234 F8.5 pc E_Zpos [] Upper value of Z interval(Z_hi) 1236-1244 F9.6 kpc d Distance (d) 1246-1254 F9.6 kpc e_d Lower value of d interval(d_lo) 1256-1265 F10.6 kpc E_d Upper value of d interval(d_hi) 1267-1285 I19 --- Source Gaia source ID (some erroneous identifiers) (source_id) 1287-1294 F8.6 --- RUWE Renormalised unit weight error (ruwe) 1296-1302 F7.3 K e_Teff Error on effective temperature (Teff_err) 1304-1308 F5.3 [cm/s2] e_logg Error on surface gravity (logg_err) 1310-1314 F5.2 --- [M/H] Metallicity ([M/H]) 1316-1323 F8.3 K Teff Effective temperature (Teff) 1325-1329 F5.3 [cm/s2] logg Surface gravity (logg) 1331-1336 F6.3 km/s vsini Rotational velocity (vsini) 1338-1341 F4.2 --- e_[M/H] Error on metallicity ([M/H]_err) -------------------------------------------------------------------------------- Acknowledgements: Madeline Lucey, m_lucey(at)utexas.edu References: Lucey et al., Paper I 2019MNRAS.488.2283L 2019MNRAS.488.2283L, Cat. J/MNRAS/488/2283 Lucey et al., Paper II 2021MNRAS.501.5981L 2021MNRAS.501.5981L, Cat. J/MNRAS/501/5981
(End) Patricia Vannier [CDS] 26-Nov-2021
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