J/AJ/167/51 Evolved Massive Stars at Low Metallicity. VI. Mass loss (Wen+, 2024)

Evolved Massive Stars at Low Metallicity. VI. Mass-loss Rate of Red Supergiant Stars in the Large Magellanic Cloud. Wen J., Gao J., Yang M., Chen B., Ren Yi, Wang T., Jiang B. <Astron. J., 167, 51 (2024)> =2024AJ....167...51W 2024AJ....167...51W
ADC_Keywords: Stars, supergiant; Photometry, infrared; Optical ; Stars, masses; Stars, diameters; Spectral types Keywords: Red supergiant stars ; Stellar mass loss ; Circumstellar dust ; Large Magellanic Cloud ; Interstellar medium Abstract: Mass loss is a crucial process that affects the observational properties, evolution path, and fate of highly evolved stars. However, the mechanism of mass loss is still unclear, and the mass-loss rate (MLR) of red supergiant stars (RSGs) requires further research and precise evaluation. To address this, we utilized an updated and complete sample of RSGs in the Large Magellanic Cloud (LMC) and employed the 2-DUST radiation transfer model and spectral energy distribution fitting approach to determine the dust-production rates (DPRs) and dust properties of the RSGs. We have fitted 4714 selected RSGs with over 100000 theoretical templates of evolved stars. Our results show that the DPR range of RSGs in the LMC is 10-11M/yr--10-7M/yr, and the total DPR of all RSGs is 1.14x10-6M/yr. We find that 63.3% RSGs are oxygen-rich, and they account for 97.2% of the total DPR. The optically thin RSG, which comprise 30.6% of our sample, contribute only 0.1% of the total DPR, while carbon-rich RSGs (6.1%) produce 2.7% of the total DPR. Overall, 208 RSGs contributed 76.6% of the total DPR. We have established a new relationship between the MLR and luminosity of RSGs in the LMC, which exhibits a positive trend and a clear turning point at logL/L∼4.4. Description: In the current work, we adopt the RSG sample from Ren+, 2021, J/ApJ/923/232, who utilized the near-infrared photometric data from UKIRT/WFCAM and the 2MASS point source catalog and astrometric data from Gaia EDR3 to identify RSGs in 12 low-mass galaxies of the Local Group. We crossmatched the RSG sample with various photometric data, including Skymapper (u, v, g, i, r, and z bands; see Wolf+ 2018, II/358), Gaia EDR3 (GBP, G, and GRP bands; Gaia Coll. 2021, I/350), Magellanic Clouds Photometric Survey (MCPS; U, B, V, and I bands; Zaritsky+ 2004, J/AJ/128/1606), Vista Magellanic Cloud Survey (VMC; Y, J, and KS bands; Cioni+ 2011, II/351), InfraRed Survey Facility (IRSF; J, H, and KS bands; Kato+ 2007, II/288), The Two Micron All Sky Survey (2MASS; J, H, and KS band; see II/246), AKARI (N3, S7, S11, L15, and L24 bands; Kato+ 2012, J/AJ/144/179), Wide field Infrared Survey Explorer (WISE; W1, W2, W3, and W4 bands; see II/328), and Spitzer ([3.6], [4.5], [5.8], [8.0], and [24] bands). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 1481 4714 *Catalog of the stellar and dust parameters for red supergiant stars in LMC -------------------------------------------------------------------------------- Note on table4.dat: Extinction correction applied to all flux values. -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/288 : IRSF Magellanic Clouds Point Source Catalog (Kato+ 2007) II/375 : VISTA Magellanic Survey (VMC) catalog (YJKs) DR6 (Cioni+, 2011) II/351 : VISTA Magellanic Survey (VMC) catalog (Cioni+, 2011) II/328 : AllWISE Data Release (Cutri+ 2013) II/358 : SkyMapper Southern Sky Survey. DR1.1 (Wolf+, 2018) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) J/ApJ/505/793 : New WR star in M33 (Massey+, 1998) J/AJ/126/2867 : Red supergiants in Magellanic Clouds (Massey+, 2003) J/AJ/128/1606 : Magellanic Clouds Photometric Survey LMC (Zaritsky+, 2004) J/A+A/442/281 : Latetype giants BVRIJHKL Teff calibration (Kucinskas+, 2005) J/A+A/503/913 : Synthetic spectrophotometry C-rich giants (Aringer+, 2009) J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009) J/AJ/142/103 : Cool evolved stars in SAGE-SMC and SAGE-LMC (Boyer+, 2011) J/ApJS/192/6 : A GALEX UV imaging survey of nearby galaxies (Lee+, 2011) J/A+A/532/A54 : GRAMS carbon-star model grid (Srinivasan+, 2011) J/ApJ/727/53 : Red supergiant stars in the LMC. I. (Yang+, 2011) J/AJ/144/179 : AKARI-LMC Point-source catalog (Kato+, 2012) J/ApJ/753/71 : Mass-loss return from LMC evolved stars. VI. (Riebel+, 2012) J/MNRAS/457/2814 : SAGE SMC evolved stars candidates (Srinivasan+, 2016) J/A+A/609/A114 : Local Group AGB stars & red supergiants (Groenewegen+, 2018) J/MNRAS/487/4832 : Period-luminosity relation red supergiants (Chatys+, 2019) J/ApJS/241/35 : Period-luminosity relationsRSGs in M33 & M31 (Ren+, 2019) J/ApJ/923/232 : Red supergiants in 12 Local Group galaxies (Ren+, 2021) J/ApJ/912/112 : Red supergiants in M31 & M33.II Mass-loss rate (Wang+, 2021) J/A+A/647/A167 : Using H-bump to identify RSGs in NGC6822 (Yang+, 2021) J/A+A/676/A84 : Mass-loss rate of RSGs in the SMC (Yang+, 2023) Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- 2MASS 2MASS Source designation 18- 20 A3 --- Type Classification of stars (always "RSG") 22- 30 F9.6 deg RAdeg [64/98] Right ascension (J2000) 32- 41 F10.6 deg DEdeg [-78/-59] Declination (J2000) 43- 53 F11.9 mag E(B-V) [0.0001/0.4] The (B-V) color excess (1) 55- 65 F11.9 mag AV [0.0006/1.24] Extinction in V band 67- 73 F7.4 mag YmagVMC [9/18.7]? VMC Y magnitude 75- 81 F7.4 mag JmagVMC [8.84/18.4]? VMC J magnitude 83- 89 F7.4 mag KsmagVMC [7.5/16.51]? VMC Ks magnitude 91- 96 F6.4 mag e_YmagVMC [0.0002/0.07]? Error in YmagVMC 98- 103 F6.4 mag e_JmagVMC [0.0002/0.1]? Error in JmagVMC 105- 110 F6.4 mag e_KsmagVMC [0.0002/0.04]? Error in KsmagVMC 112- 117 F6.3 mag Jmag2MASS [7.75/13.3] 2MASS J magnitude 119- 124 F6.3 mag Hmag2MASS [6.96/12.4] 2MASS H magnitude 126- 131 F6.3 mag Kmag2MASS [6.55/12.1] 2MASS Ks magnitude 133- 138 F6.4 mag e_Jmag2MASS [0.005/0.1] Error in Jmag2MASS 140- 145 F6.4 mag e_Hmag2MASS [0.01/0.1] Error in Hmag2MASS 147- 152 F6.4 mag e_Kmag2MASS [0.007/0.1] Error in Ksmag2MASS 154- 162 F9.6 mag GBPmag [11/18.5]? Gaia EDR3 GBP magnitude 164- 172 F9.6 mag Gmag [10.49/16.55]? Gaia EDR3 G magnitude 174- 182 F9.6 mag GRPmag [9.48/15.2]? Gaia EDR3 GRP magnitude 184- 191 F8.6 mag e_GBPmag [0.0028/0.1]? Error in GBPmag 193- 200 F8.6 mag e_Gmag [0.0027/0.07]? Error in Gmag 202- 209 F8.6 mag e_GRPmag [0.0037/0.1]? Error in GRPmag 211- 216 F6.3 mag gmagS [10.76/18.65]? Skymapper g magnitude 218- 223 F6.3 mag rmagS [10.33/18.12]? Skymapper r magnitude 225- 230 F6.3 mag imagS [9.58/16.21]? Skymapper i magnitude 232- 237 F6.3 mag zmagS [9.3/15.1]? Skymapper z magnitude 239- 244 F6.3 mag umagS [11.85/18.63]? Skymapper u magnitude 246- 251 F6.3 mag vmagS [11.72/18.3]? Skymapper v magnitude 253- 257 F5.3 mag e_gmagS [0.002/0.1]? Error in gmagS 259- 263 F5.3 mag e_rmagS [0.002/0.1]? Error in rmagS 265- 269 F5.3 mag e_imagS [0.002/0.1]? Error in imagS 271- 275 F5.3 mag e_zmagS [0.002/0.1]? Error in zmagS 277- 281 F5.3 mag e_umagS [0.002/0.1]? Error in umagS 283- 287 F5.3 mag e_vmagS [0.003/0.1]? Error in vmagS 289- 297 F9.6 mag mag36 [6.27/12.51]? Spitzer 3.6 micron magnitude 299- 307 F9.6 mag mag45 [6.12/12.5]? Spitzer 4.5 micron magnitude 309- 317 F9.6 mag mag58 [5.72/12.4]? Spitzer 5.8 micron magnitude 319- 327 F9.6 mag mag80 [4.87/12.4]? Spitzer 8.0 micron magnitude 329- 334 F6.3 mag mag24 [2.54/11.1]? Spitzer 24 micron magnitude 336- 340 F5.3 mag e_mag36 [0.018/0.2]? Error in mag36 342- 346 F5.3 mag e_mag45 [0.015/0.2]? Error in mag45 348- 352 F5.3 mag e_mag58 [0.016/0.2]? Error in mag58 354- 358 F5.3 mag e_mag80 [0.013/0.2]? Error in mag80 360- 364 F5.3 mag e_mag24 [0.006/0.3]? Error in mag24 366- 371 F6.3 mag W1mag [6.3/12.24]? WISE W1 magnitude 373- 378 F6.3 mag W2mag [6.2/12.32]? WISE W2 magnitude 380- 385 F6.3 mag W3mag [4.39/12.5]? WISE W3 magnitude 387- 391 F5.3 mag W4mag [3.36/8.591]? WISE W4 magnitude 393- 397 F5.3 mag e_W1mag [0.018/0.05]? Error in W1mag 399- 403 F5.3 mag e_W2mag [0.018/0.04]? Error in W2mag 405- 409 F5.3 mag e_W3mag [0.013/0.2]? Error in W3mag 411- 415 F5.3 mag e_W4mag [0.018/0.2]? Error in W4mag 417- 422 F6.3 mag N3mag [6.51/12.1]? AKARI N3 magnitude 424- 429 F6.3 mag S7mag [5.3/12.21]? AKARI S7 magnitude 431- 436 F6.3 mag S11mag [3.5/12.1]? AKARI S11 magnitude 438- 442 F5.3 mag L15mag [3.51/9.92]? AKARI L15 magnitude 444- 448 F5.3 mag L24mag [2.56/8.5]? AKARI L24 magnitude 450- 454 F5.3 mag e_N3mag [0.014/0.1]? Error in N3mag 456- 460 F5.3 mag e_S7mag [0.003/0.1]? Error in S7mag 462- 466 F5.3 mag e_S11mag [0.002/0.1]? Error in S11mag 468- 472 F5.3 mag e_L15mag [0.024/0.1]? Error in L15mag 474- 478 F5.3 mag e_L24mag [0.01/0.1]? Error in L24mag 480- 484 F5.2 mag JmagIRSF [8.66/13.66]? IRSF J magnitude 486- 490 F5.2 mag HmagIRSF [8.43/12.77]? IRSF H magnitude 492- 496 F5.2 mag KsmagIRSF [8.87/12.83]? IRSF Ks magnitude 498- 501 F4.2 mag e_JmagIRSF [0.01/0.08]? Error in JmagIRSF 503- 506 F4.2 mag e_HmagIRSF [0.01/0.07]? Error in HmagIRSF 508- 511 F4.2 mag e_KsmagIRSF [0.01/0.09]? Error in KsmagIRSF 513- 518 F6.3 mag Umag [10.74/20.9]? MCPS U magnitude 520- 525 F6.3 mag Bmag [11.75/20.5]? MCPS B magnitude 527- 532 F6.3 mag Vmag [11.4/19.22]? MCPS V magnitude 534- 539 F6.3 mag Imag [8.84/16.71]? MCPS I magnitude 541- 545 F5.3 mag e_Umag [0.01/0.1]? Error in Umag 547- 551 F5.3 mag e_Bmag [0.01/0.1]? Error in Bmag 553- 557 F5.3 mag e_Vmag [0.01/0.1]? Error in Vmag 559- 563 F5.3 mag e_Imag [0.02/0.1]? Error in Imag 565- 575 F11.9 Jy flux2massJ [0.008/1.3] 2MASS J band flux 577- 587 F11.9 Jy flux2massH [0.01/1.7] 2MASS H band flux 589- 599 F11.9 Jy flux2massKs [0.009/1.6] 2MASS Ks band flux 601- 611 F11.9 Jy e_flux2massJ [0.0001/0.03] Error in flux2massJ 613- 623 F11.9 Jy e_flux2massH [0.0002/0.06] Error in flux2massH 625- 635 F11.9 Jy e_flux2massKs [0.0001/0.04] Error in flux2massKs 637- 647 F11.9 Jy fluxGBP [0.0001/0.2]? Gaia BP band flux 649- 659 F11.9 Jy fluxGRP [0.002/0.5]? Gaia RP band flux 661- 671 F11.9 Jy fluxG [0.0007/0.3]? Gaia G band flux 673- 680 E8.2 Jy e_fluxG [2.6e-06/0.002]? Error in fluxG 682- 689 E8.2 Jy e_fluxGBP [1.4e-06/0.004]? Error fluxGBP 691- 698 E8.2 Jy e_fluxGRP [1e-05/0.008]? Error in fluxGRP 700- 710 F11.9 Jy flux36 [0.002/0.9]? Spitzer 3.6 micron band flux 712- 722 F11.9 Jy flux45 [0.0019/0.7]? Spitzer 4.5 micron band flux 724- 734 F11.9 Jy flux58 [0.001/0.6]? Spitzer 5.8 micron band flux 736- 746 F11.9 Jy flux80 [0.0007/0.8]? Spitzer 8.0 micron band flux 748- 758 F11.9 Jy flux24 [0.0002/0.7]? Spitzer 24 micron band flux 760- 770 F11.9 Jy e_flux36 [0.0001/0.04]? Error in flux36 772- 779 E8.2 Jy e_flux45 [5e-05/0.03]? Error in flux45 781- 788 E8.2 Jy e_flux58 [4.9e-05/0.03]? Error in flux58 790- 797 E8.2 Jy e_flux80 [3.3e-05/0.03]? Error in flux80 799- 806 E8.2 Jy e_flux24 [3.8e-05/0.004]? Error in flux24 808- 818 F11.9 Jy fluxW1 [0.0039/1]? WISE W1 band flux 820- 830 F11.9 Jy fluxW2 [0.002/0.6]? WISE W2 band flux 832- 842 F11.9 Jy fluxW3 [0.0003/0.6]? WISE W3 band flux 844- 854 F11.9 Jy fluxW4 [0.003/0.4]? WISE W4 band flux 856- 863 E8.2 Jy e_fluxW1 [8.5e-05/0.05]? Error in fluxW1 865- 872 E8.2 Jy e_fluxW2 [4e-05/0.02]? Error in fluxW2 874- 881 E8.2 Jy e_fluxW3 [3e-05/0.008]? Error in fluxW3 883- 893 F11.9 Jy e_fluxW4 [0.0002/0.008]? Error in fluxW4 895- 902 E8.2 Jy fluxSu [4.6e-05/0.03]? Skymapper u band flux 904- 911 E8.2 Jy e_fluxSu [6e-07/0.0005]? Error in fluxSu 913- 923 F11.9 Jy fluxSv [0.0001/0.06]? Skymapper v band flux 925- 932 E8.2 Jy e_fluxSv [1.6e-06/0.002]? Error in fluxSv 934- 944 F11.9 Jy fluxSg [0.0001/0.2]? Skymapper g band flux 946- 953 E8.2 Jy e_fluxSg [2.7e-06/0.004]? Error in fluxSg 955- 965 F11.9 Jy fluxSi [0.0008/0.4]? Skymapper i band flux 967- 974 E8.2 Jy e_fluxSi [4e-06/0.006]? Error in fluxSi 976- 986 F11.9 Jy fluxSr [0.00018/0.3]? Skymapper r band flux 988- 998 F11.9 Jy e_fluxSr [3e-06/0.006]? Error in fluxSr 1000- 1010 F11.9 Jy fluxSz [0.002/0.5]? Skymapper z band flux 1012- 1019 E8.2 Jy e_fluxSz [6e-06/0.008]? Error in fluxSz 1021- 1031 F11.9 Jy fluxN3 [0.005/0.9]? AKARI N3 band flux 1033- 1040 E8.2 Jy e_fluxN3 [8.6e-05/0.05]? Error in fluxN3 1042- 1052 F11.9 Jy fluxS7 [0.0009/0.6]? AKARI S7 band flux 1054- 1061 E8.2 Jy e_fluxS7 [4e-05/0.002]? Error in fluxS7 1063- 1073 F11.9 Jy fluxS11 [0.0005/1.4]? AKARI S11 band flux 1075- 1082 E8.2 Jy e_fluxS11 [3.8e-05/0.009]? Error in fluxS11 1084- 1094 F11.9 Jy fluxL15 [0.0017/0.7]? AKARI L15 band flux 1096- 1106 F11.9 Jy e_fluxL15 [0.0001/0.05]? Error in fluxL15 1108- 1118 F11.9 Jy fluxL24 [0.0029/0.7]? AKARI L24 band flux 1120- 1130 F11.9 Jy e_fluxL24 [0.0002/0.01]? Error in fluxL24 1132- 1142 F11.9 Jy fluxvmcY [0.004/0.4]? VMC Y band flux 1144- 1151 E8.2 Jy e_fluxvmcY [4.4e-6/9.2e-5]? Error in fluxvmcY 1153- 1163 F11.9 Jy fluxvmcJ [0.01/0.4]? VMC J band flux 1165- 1172 E8.2 Jy e_fluxvmcJ [4.9e-06/0.0002]? Error in fluxvmcJ 1174- 1184 F11.9 Jy fluxvmcKs [0.008/0.3]? VMC Ks band flux 1186- 1193 E8.2 Jy e_fluxvmcKs [4.9e-6/0.0002]? Error in fluxvmcKs 1195- 1202 E8.2 Jy fluxU [8e-06/0.1]? MCPS U band flux 1204- 1211 E8.2 Jy e_fluxU [7.4e-07/0.0009]? Error in fluxU 1213- 1223 F11.9 Jy fluxV [7.5e-05/0.1]? MCPS V band flux 1225- 1232 E8.2 Jy e_fluxV [5.5e-06/0.005]? Error in fluxV 1234- 1244 F11.9 Jy fluxB [2.6e-05/0.08]? MCPS B band flux 1246- 1253 E8.2 Jy e_fluxB [1.7e-06/0.0008]? Error in fluxB 1255- 1265 F11.9 Jy fluxI [0.0004/0.7]? MCPS I band flux 1267- 1277 F11.9 Jy e_fluxI [4.5e-05/0.05]? Error in fluxI 1279- 1289 F11.9 Jy fluxirsfJ [0.005/0.6]? IRSF J band flux 1291- 1301 F11.9 Jy e_fluxirsfJ [6e-05/0.02]? Error in fluxirsfJ 1303- 1313 F11.9 Jy fluxirsfH [0.008/0.5]? IRSF H band flux 1315- 1325 F11.9 Jy e_fluxirsfH [7.4e-05/0.02]? Error in fluxirsfH 1327- 1337 F11.9 Jy fluxirsfKs [0.0049/0.2]? IRSF K band flux 1339- 1349 F11.9 Jy e_fluxirsfKs [5.9e-05/0.02]? Error in fluxirsfKs 1351- 1361 F11.9 --- chi [0.003/0.8] Lowest chi-squared value for best-fitting model 1363- 1366 I4 K Teff [2600/5000] Best-fitting effective temperature 1368- 1374 F7.5 --- tau [0.0001/2] Best-fitting optical depth 1376- 1378 A3 --- mType Chemical type of best-fitting model (2) 1380- 1385 I6 Lsun lum [1670/386000] Model luminosity output from 2-DUST 1387- 1393 F7.3 [Msun/yr] log(DPR) [-12.71/-7.5] Log of best-fitting dust production rate 1395- 1399 I5 yr time [776/63000] Time scale for mass loss or dust production 1401- 1408 E8.2 Msun massDust [2.5e-10/0.0004] Total mass of dust shell 1410- 1417 E8.2 g/cm3 density [2.3e-23/3e-18] Density of dust at inner radius 1419- 1426 E8.2 cm Rstar [8170000000000/79600000000000] Star radius of best-fitting photosphere model 1428- 1432 I5 --- index [330/72363] Specific index number in model library corresponding to best-fitting RSG model 1434- 1437 F4.1 [-] log(g) [-0.5/0] Log of surface gravity of best-fitting photosphere model 1439- 1442 F4.1 [-] [M/H] [-0.5/0] Metallicity of best- fitting photosphere model 1444- 1447 F4.1 Msun mass [0.5/15] Mass of best-fitting photosphere model 1449- 1451 F3.1 --- sType [0/3] Classification of source (3) 1453- 1459 F7.3 [Msun/yr] log(DPRv) [-13.2/-7.6] Log of scaled DPR 1461- 1466 F6.3 km/s v [3/12] Scaled wind speed of dust shell 1468- 1469 I2 --- Rmin [3/25] Inner radius in units of stellar radius 1471- 1475 F5.3 [Lsun] log(lumobs) [3.29/5.52] Log of integrated luminosity obtained from observed SED 1477- 1481 F5.3 [Lsun] log(lummod) [3.2/5.6] Log of integrated luminosity obtained from best- fitting model SED -------------------------------------------------------------------------------- Note (1): The E(B-V) values come from the extinction map of Chen et al. (2022). Note (2): Types as followd: C = carbon-rich model; O = oxygen-rich model; Opt = optically thin model. Note (3): Classification as follows: 0.0 = normal source; 2.0 = contamination or binarity; 2.5 = slight flux excess source; 3.0 = source with bad W3 or W4 data. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Yang et al. Paper I : 2019A&A...629A..91Y 2019A&A...629A..91Y Cat. J/A+A/629/A91 Yang et al. Paper II : 2020A&A...639A.116Y 2020A&A...639A.116Y Cat. J/A+A/639/A116
(End) Prepared by [AAS], Coralie fix [CDS], 03-Jun-2024
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