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Home All issues Volume 688 (August 2024) A&A, 688 (2024) A105 Full HTML
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Table A.1

Stellar parameters and spectral types from ULLYSES metadata along with terminal wind speeds for supergiants in the LMC.

ID Sp. Type log(LL⊙)$\log ({L \over {{L_ \odot }}})$ ΔL Teff ΔTeff v∞(DM) Δv v∞(SEI) Δv vturb Δv Mevol ΔMevol vesc Δvesc Q Alias Ref
[dex] [kK] [km s−1] [km s−1] [km s−1] [M⊙] [km s−1]
Sk −67° 22 O2 If*/WN5 5.8 0.1 50 2.4 2900 20 2590 30 430 30 61 8 1480 130 i BAT99-12 18
BAT99-105 O2 If* 6.56 0.1 47.3 2.4 2920 100 2930 30 300 20 153 43 1500 240 ii Mk 42 19
VFTS 482 O2.5 If*/WN6 6.4 0.1 42.2 2.1 2420 100 2530 30 560 30 111 22 1220 160 ii Mk 39, BAT99-99 19
VFTS 180 O3 If* 5.92 0.1 42.2 2.1 2160 60 2170 30 180 20 57 8 1180 120 i BAT99-93, ST921-78 19
Sk −65° 47 O4 If 5.98 0.2 40.5 2.7 2180 110 1960 30 430 20 37 9 910 170 i 15
Sk −71° 46 O4 If 6.1 0.1 38 2.1 2490 70 2160 10 540 0 68 11 1030 120 i NGC206 FS 214 23
Sk −67° 167 O4 Inf+ 5.87 0.2 40.1 4.0 2420 60 2130 40 530 50 47 11 1180 240 i 1
ST92 4-18 O5 If 5.61 0.2 38.3 2.0 2460 80 2320 40 280 30 34 6 1080 180 i W61 4-4 1
LMCE078-1 O6 Ifc 5.6 0.2 36.4 2.2 2330 70 2240 40 560 40 32 6 980 170 i 1
Sk −67º 111 O6 Ia(n)fpv 5.74 0.2 36.4 2.3 1970 20 1690 30 350 30 37 8 960 170 i 1
Sk −70° 115 O6 If 6.02 0.2 36.4 2.0 2110 10 1840 50 460 50 50 13 950 180 i HDE 270145 1
Sk −69° 104 O6 Ib(f) 5.94 0.2 36.4 2.1 2460 100 2660 60 520 40 47 11 990 180 ii HDE 269357 1
Sk −65° 22 06 Iaf+ 5.86 0.1 33.5 2.0 1510 100 1330 30 330 30 48 6 900 100 i
Sk −69° 50 O7(n)(f)p 5.5 0.2 36.1 2.0 1890 40 1700 30 420 30 28 5 930 150 i 1
Sk −67° 168 O8 I(f)p 5.84 0.2 32.6 1.2 1960 50 1780 20 380 20 39 10 830 150 i HDE 269702 1
LH 9-34 O8.5 Iaf 5.67 0.2 31.7 3.2 1510 100 1470 40 370 30 32 7 830 170 i PGMW 1363, BI37 1
Sk −67° 107 O9 Ib(f) 5.61 0.2 30.7 1.9 1840 10 1810 30 420 30 30 7 780 140 i 1
Sk −69° 279 O9.2 Iaf 5.54 0.1 29.5 1.7 460 100 620 10 150 10 32 4 770 80 ii 25
Sk −7lº 4l O9.7 lab 5.5 0.1 30 1.7 1710 30 1660 40 360 40 30 3 780 80 i NGC206 FS 134 23
Sk −67° 5 O9.7 lb 6.04 0.2 29.4 1.2 1490 100 1320 40 330 40 49 14 750 140 i HDE 268605 1
VFTS 87 O9.7 Ib-II 5.29 0.2 30.5 2.9 1010 190 1550 100 390 120 21 3 850 180 ii 22
Sk −68° 135 ON9.7 Ia+ 5.97 0.1 27.5 0.7 810 60 970 20 240 20 52 7 710 70 i HDE 269896 3
Sk −68° 52 B0 la 5.76 0.1 24.5 2.2 1080 100 1170 20 290 20 39 5 640 90 i HDE 269050 3
Sk −68° 155 B0.5 I 5.51 0.2 25.4 1.4 1630 100 1530 0 380 20 25 5 620 100 i 1
Sk −68° 140 B0.7 Ib-IabNwk 5.64 0.1 23.5 1.7 890 100 1150 0 230 0 33 4 610 80 i VFTS 696 20
Sk −66° 35 BCl Ia 5.73 0.1 22 1.1 490 100 810 50 200 30 37 9 810 280 i HDE 268723 21
Sk −68° 129 B1 I 5.25 0.2 22.2 2.2 1300 100 1380 40 340 30 23 5 620 130 ii W6l 27-56 1+
Sk −67° 2 B1 Ia+ 5.92 0.1 19.92 2.4 320 100 480 20 120 10 51 8 490 80 ii HDE 270754 21
Sk −67° 14 Bl.5 Ia 5.74 0.1 22.89 2.6 910 100 900 10 220 10 37 5 600 100 i HDE 268685 21
Sk −68° 26 BC2 Ia 5.71 0.1 18.16 1.4 250 140 390 0 100 0 38 4 430 50 i 24
Sk −69° 140 B4 I 4.73 0.2 15 1.9 890 100 1130 10 160 10 11 2 540 60 ii 1
Sk −70° 16 B4 I 4.62 0.2 15 2.4 910 100 1010 10 110 10 11 2 580 70 ii 1
NGC2004 ELS 3 B5 Ia 5.1 0.2 14.45 1.6 400 100 440 10 110 10 41 9 1080 180 ii R109 12
Sk −68° 8 B5 Ia+ 5.54 0.2 14.2 2.4 270 100 300 0 20 0 40 4 410 110 iv HDE 268729 1

Reference 1 indicates the stellar parameters come from spectral type calibrations. The addition of the plus sign indicates this star was not in the original ULLYSES sample, but has been added from archival spectra. Further numbers indicate the source of the stellar parameters from 2 Crowther et al. 2002, 3 Evans et al. 2004, 4 Walborn et al. 2004, 5 Trundle et al. 2004, 6 Massey et al. 2004, 7 Trundle & Lennon 2005, 8 Dufton et al. 2005, 9 Massey et al. 2005, 10 Hunter et al. 2005, 11 Heap et al. 2006, 12 Trundle et al. 2007, 13 Hunter et al. 2007, 14 Massey et al. 2009, 15 Rivero González et al. 2012, 16 Massey et al. 2013, 17 Bouret et al. 2013, 18 Hainich et al. 2014, 19 Bestenlehner et al. 2014, 20 McEvoy et al. 2015, 21 Urbaneja et al. 2017, 22 Ramírez-Agudelo et al. 2017, 23 Ramachandran et al. 2018, 24 Urbaneja et al. 2018, 25 Gvaramadze et al. 2018, 26 Castro et al. 2018, 27 Dufton et al. 2019, 28 Mahy et al. 2020, 29 Bouret et al. 2021, and 30 Pauli et al. 2022

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