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## (from tabmap V6.0 (2016-08-18)) 2024-05-09T16:19:14 #--------------------------------------------------------------------------- #-- J/AJ/118/1684 UBV photometry of 4 LMC compact OB groups (Walborn+, 1999) #-------------------------------------------------------------------------- #---Table: J/AJ/118/1684/./table3.dat Observed and derived parameters for the components of LH 10-3209 (6 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 --|------|------|-----|-|-----|-----|-----|-|-----|------|-----|---------------|-|--------------- 17|584.15|102.76|12.73| |-0.07|-1.13| 0.25| |4.707|-11.17|-4.56|O3 III(f*) | |Star A 18|584.53|105.73|14.26| | 0.07|-0.20| 0.38| |4.555| -8.95|-3.48|O9 V | |Star B 14|573.82|100.73|14.49| | 0.04|-1.28| 0.36| |4.613| -9.07|-3.89|O7 V | |Star C 16|575.74|100.70|15.57|e| | | 0.32|e|4.555| -7.47|-3.48|O9 V | |Star E 15|574.46| 96.60|15.76| | 0.00|-0.82| 0.30| |4.539| -7.10|-3.37|O9.5 V | |Star D 19|595.06| 94.66|15.88| | 0.00|-0.90| 0.30| |4.539| -6.98|-3.37|O9.5 V | |Star F -------------------------------------------------------------------------------------------------