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## (from tabmap V6.0 (2016-08-18)) 2024-05-13T02:54:26 #--------------------------------------------------------------------------- #-- J/AJ/118/1684 UBV photometry of 4 LMC compact OB groups (Walborn+, 1999) #-------------------------------------------------------------------------- #---Table: J/AJ/118/1684/./table2.dat Observed and derived parameters for the components of NGC 2044 West (38 records) #------------------------------------------------------------------------------- # Label Format Unit Explanations #------------------------------------------------------------------------------- # Seq I2 --- Sequential number (1) # Xpos F6.2 pix X position (1) # Ypos F6.2 pix Y position (1) # Vmag F5.2 mag HST/WFPC F569W V magnitude # n_Vmag A1 --- [e] discrepant photometry (2) # B-V F5.2 mag ? B-V colour index (F439W-F569W) # U-B F5.2 mag ? U-B colour index (F336W-F439W) # E(B-V) F5.2 mag ? B-V colour excess # n_E(B-V) A1 --- [ce] discrepant photometry (2) # logTe F5.3 [K] ? Effective temperature # Mbol F6.2 mag ? Bolometric magnitude # BC F5.2 mag ? Bolometric correction # SpType A15 --- MK spectral type (3) # n_SpType A1 --- [d] Note (3) # ID A15 --- Alternate ID (4) #------------------------------------------------------------------------------- #Note (1): Running number and detector coordinates from the present photometry, # to be presented in full by Parker et al. in a subsequent paper. # * In table1: <Brey 73 NN> in Simbad # * In table2: <NGC 2044W NN> in Simbad # * In table3: <LH 10-3209 NN> in Simbad # * In table4: <HD 32228 NN> in Simbad #Note (2): Notes as follows: # c = The colors for these components were discrepant, so the average # color excess of the other spectroscopically classified # components was adopted instead # e = The photometry for this component was discrepant, so the magnitude # difference from component C in the V deconvolution and the average # color excess of the other components were adopted for it instead. #Note (3): Spectroscopy from HST Faint Object Spectrograph, unless # d = Spectral type from Schild & Testor (1992A&AS...92..729S) or # Heydari-Malayeri et al. (1993A&A...278...11H) #Note (4): Alternative IDs refer to: # * Table1: # Tes = Testor et al. (1988Msngr..54...43T) with letters added # here to the numbers to denote subsequently resolved components. # * Table2: # H-M = Heydari-Malayeri et al. (1993 A&A...278...11H) with letters # added here to the numbers to denote subsequently resolved # components. # * Table3: See fig. 9 of the paper # * Table4: # Sch = Schertl et al. (1995A&A...302..327S) # H-M = Heydari-Malayeri et al. (1983A&A...118..116H) # with arabic numerals added here to the letters to denote # subsequently resolved components. #------------------------------------------------------------------------------- ------------------------------------------------------------------------------------------------- | | | | | | | |n| | | | |n| | | | | | | | |_| | | | |_| | | | |n| | | |E| | | | |S| | | | |_| | | |(| | | | |p| | | | |V| | | |B| | | | |T| | | | |m| | | |-| | | | |y| S| | | |a| | | E|V| | | | |p| eq| Xpos| Ypos| Vmag|g| B-V| U-B|(B-V)|)|logTe| Mbol| BC|SpType |e|ID --|------|------|-----|-|-----|-----|-----|-|-----|------|-----|---------------|-|--------------- 36|154.69|174.32|13.09| | 0.02|-0.93| | | | | |WN7 | |Brey 65 40|157.79|241.41|13.42| | | | 0.36| |4.678|-10.61|-4.35|O4 If+ | |H-M 9A 24|131.03|201.21|13.96| | | | 0.36| |4.476| -8.76|-3.03|B0 I | |H-M 5Aa 35|154.70|227.01|14.01| | 0.01|-1.03| 0.33| |4.683| -9.97|-4.39|O4 III | |H-M 7 13|112.79|180.69|14.14| | 0.04|-0.92| 0.35| |4.585| -9.21|-3.69|O8 V | |H-M 6 42|162.21|217.85|14.30| | 0.01|-0.88| 0.32| |4.569| -8.84|-3.58|O8 III | |H-M 8 26|132.13|199.62|14.45| | 0.06|-0.75| 0.36| |4.438| -8.04|-2.81| | |H-M 5B 27|133.74|197.54|14.59| | 0.01|-0.53| | | | | |WN4(h) | |H-M 5C 23|130.83|200.29|14.84| |-0.02|-1.14| 0.36| |4.667| -9.12|-4.28| | |H-M 5Ab 41|160.60|239.39|14.88| |-0.01|-0.13| 0.36| |4.034| -5.21|-0.41| | |H-M 9B 1| 58.88|207.25|15.00| | 0.09|-0.84| 0.36| |4.537| -8.03|-3.35| | | 29|135.41|237.25|15.15| | 0.09|-0.74| 0.41| |4.599| -8.48|-3.79|O7.5 V | |H-M 11A 8|100.32|221.51|15.21| | 0.08|-0.87| 0.40| |4.652| -8.76|-4.17|O5.5 V | |H-M 20 33|145.55|193.95|15.32| | 0.04|-0.90| 0.35| |4.555| -7.81|-3.48|O9 V | |H-M 3 28|134.62|200.39|15.39| | 0.51|-1.05| 0.36| |3.913| -4.27| 0.02| | |H-M 5E 16|120.21|246.67|15.40| | 0.13|-0.83| 0.36| |4.555| -7.76|-3.48| | | 9|101.94|204.22|15.42| | 0.03|-0.86| 0.36| |4.516| -7.46|-3.20| | | 39|157.18|238.34|15.68| | 0.66| 0.17| 0.36| |3.856| -3.94| 0.06| | | 30|136.70|236.23|15.77| | 0.14| 0.21| 0.36| |4.315| -5.99|-2.08| | |H-M 11B 45|176.86|264.93|15.88| |-0.02|-0.80| 0.36| |4.432| -6.57|-2.77| | | 20|126.57|199.87|15.91| | 0.19|-1.16| 0.36| |4.204| -5.19|-1.42| | |H-M 5D 34|153.51|198.74|16.38| |-0.08|-0.71| 0.36| |4.326| -5.44|-2.14| | | 43|165.74|265.81|16.41| | 0.25|-0.78| 0.36| |4.072| -3.91|-0.64| | | 7| 92.10|201.15|16.77| |-0.06|-0.43| 0.36| |4.154| -4.03|-1.12| | | 25|131.59|216.87|16.79| |-0.14|-0.74| 0.36| |4.316| -4.98|-2.08| | | 44|166.39|235.85|16.88| | 0.08|-0.88| 0.36| |4.568| -6.37|-3.57| | | 37|156.51|286.85|16.90| | 0.67|-1.24| 0.36| |3.853| -2.72| 0.06| | | 3| 80.34|224.85|16.97| | 0.04|-0.77| 0.36| |4.443| -5.54|-2.83| | | 14|113.16|209.92|17.00| | 0.01|-0.70| 0.36| |4.368| -5.07|-2.39| | | 31|139.30|215.80|17.05| | 0.16|-0.78| 0.36| |4.528| -5.92|-3.29| | | 22|129.73|263.86|17.34| |-0.13|-0.08| 0.36| |4.910| -8.33|-5.99| | | 38|156.60|286.17|17.42| | 0.26|-0.44| 0.36| |4.307| -4.29|-2.03| | | 21|129.73|252.95|17.54| | 0.00|-0.76| 0.36| |4.410| -4.78|-2.64| | | 19|126.38|307.92|17.60| | 0.43|-0.47| 0.36| |3.954| -2.15|-0.07| | | 12|110.68|294.95|17.68| | 0.34|-0.73| 0.36| |3.874| -1.94| 0.06| | | 17|120.58|207.32|17.74| | 0.21|-1.05| 0.36| |4.160| -3.10|-1.16| | | 10|104.43|216.00|18.16| | 0.05|-0.21| 0.36| |4.083| -2.23|-0.70| | | 18|125.87|218.97|18.23| |-0.35|-0.91| 0.36| |4.330| -3.62|-2.17| | | -------------------------------------------------------------------------------------------------