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 نام B F HD HIP بعد میل vis.mag. abs.mag. فاصله (ly) رده‌بندی یادداشت Canopus  α    45348  30438      −0.72  −5.53  313  F0Ib  Suhel; 2nd brightest star, nearest supergiant β Car  β    80007  45238      1.67  −0.99  111  A2IV  Miaplacidus ε Car  ε    71129  41037      1.86  −4.58  632  K3III+B2V  Avior; suspected eclipsing binary,  ι Car  ι    80404  45556      2.23  −4.43  692  A8Ib  Aspidiske, Turais, Scutulum; suspected variable,  θ Car  θ    93030  52419      2.74  −2.91  439  B0Vp  in IC 2602 υ Car  υ    85123  48002      2.92  −5.56  1622  A9  binary star ω Car  ω    89080  50099      3.29  −1.99  370  B8III   p Car  p  PP  91465  51576      3.30  −2.62  497  B4Vne  γ Cas variable,  V337 Car  q  V337  89388  50371      3.39  −3.38  736  K3II  irregular variable,  a Car  a  V357  79351  45080      3.43  −2.11  418  B2IV  eclipsing binary,  χ Car  χ    65575  38827      3.46  −1.91  387  B3IVp  β Cep variable,  l Car  l    84810  47854      3.69  −4.64  1509  G5Iab/Ib  classical Cepheid,  HD 94510  u    94510  53253      3.78  1.42  97  K0III-IV...  suspected variable,  HD 90853  s    90853  51232      3.81  −3.71  1042  F2II  suspected variable HD 76728  c    76728  43783      3.84  −1.06  312  B8III  double star V382 Car  x  V382  96918  54463      3.93  −7.37  5927  G0Ia0  hypergiant; slow irregular variable,  HD 79447  i    79447  45101      3.96  −1.97  499  B3IV  variable star,  HD 90589  I    90589  50954      3.99  2.94  53  F2IV  suspected variable,  HD 83183  h    83183  46974      4.08  −4.83  1976  B5II  V343 Car  d  V343  74375  42568      4.31  −3.87  1411  B1.5III  β Cep variable HD 80230  g    80230  45496      4.34  −1.74  536  M1III  suspected variable,  HD 47306  N    47306  31407      4.35  −4.31  1762  B9III  HR 2554  A  V415  50337  32761      4.39  −1.74  553  G6II  Algol variable,  HD 91942  r    91942  51849      4.45  −3.68  1376  K3/K4II  suspected variable η Car  η    93308        4.47    7500  LBV  Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, ; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known. HR 3643  G    78791  44599      4.47  −1.25  454  F6II-III  V344 Car  f  V344  75311  43105      4.50  −1.62  546  B3Vne  γ Cas variable,  HD 83944  m    83944  47391      4.51  0.33  224  B9V  suspected variable V520 Car  w  V520  93070  52468      4.58  −2.99  1065  K3Ib  irregular variable,  V533 Car  y  V533  97534  54751      4.59  −8.34  12538  A6Ia  α Cyg variable HD 96566  z1    96566  54301      4.62  −0.65  370  G8III  V399 Car  P  V399  90772  51192      4.65      A6Ia  semiregular variable,  V345 Car  E  V345  78764  44626      4.67  −2.94  1079  B2IVe  γ Cas variable,   HD 92397   t2    92397  52102      4.69  −4.08  1852  K4/K5III:  suspected variable HD 91375  K    91375  51438      4.72  0.22  259  A2III  HR 3220  B    68456  39903      4.74  3.09  70  F5V  V518 Car    V518  92938  52370      4.76  −0.97  456  B3V  in IC 2602; γ Cas variable HD 81101  k    81101  45856      4.79  0.62  223  G6III  HD 93194      93194  52502      4.80  −1.06  484  B5Vn  in IC 2602; suspected irregular variable,  HD 66591  D    66591  39138      4.81  −1.29  542  B3V  suspected variable HD 73389  e2    73389  42134      4.84  0.60  229  K0III  HD 93607      93607  52736      4.87  −0.83  449  B3IV  in IC 2602; suspected variable HD 61248  Q    61248  36942      4.93  −0.48  394  K3III  suspected variable V376 Car  b1  V376  77002  43937      4.93  −1.47  621  B2IV-V  β Cep variable,  HD 91496      91496  51495      4.94  −2.42  964  K4/K5III  suspected variable,  HD 90264  L    90264  50847      4.97  −0.63  430  B8V  HD 92063  t1    92063  51912      5.08  0.50  269  K1III  HD 59219      59219  36114      5.09  −1.09  562  K0III  HD 96919  z2  V371  96919  54461      5.12  −6.03  5525  B9Ia  α Cyg variable,  HD 53047      53047  33779      5.14  −1.25  617  M1III  semiregular variable V386 Car    V386  54118  34105      5.14  0.45  282  A0p:  α2 CVn variable,  HD 88981  M    88981  50083      5.15  0.31  304  Am  HD 69863  C    69863  40429      5.16  0.81  242  A+...  binary star HD 77370  b2    77370  44143      5.17  3.08  85  F3V  HR 3153    V460  66342  39070      5.19  −2.34  1045  M0II  in NGC 2516; semiregular variable,  HD 97583      97583  54767      5.22  0.30  314  B9V  double star HD 93549      93549  52701      5.23  −0.37  429  B7IV  in IC 2602 HD 88323      88323  49698      5.26  0.16  341  K0III  optical double V524 Car    V524  94367  53154      5.26  −6.08  6037  B9Ia  α Cyg variable HD 73390  e1    73390  42129      5.27  −2.08  962  B3V+...  HD 91056      91056  51313      5.27  −4.64  3135  K3Ib  slow irregular variable HD 80951      80951  45581      5.28  −1.44  721  A1V  HD 84121      84121  47479      5.30  1.16  220  A3IV  HD 93540      93540  52678      5.33  −0.45  466  B7:V  in IC 2602; suspected variable HD 92964    V519  92964  52405      5.36  −6.23  6792  B2.5Ia  α Cyg variable,  HD 57917      57917  35589      5.38  −0.52  493  B9V  HD 80671      80671  45571      5.38  2.75  109  F4V  HD 49689      49689  32494      5.39  −1.83  906  K1II/IIIp+G:  suspected variable HD 73887      73887  42286      5.45  0.39  335  K0III  HD 82350      82350  46358      5.46  1.51  201  K2III  HD 83095  H    83095  46741      5.46  −1.47  791  K4III  HD 92207    V370  92207  52004      5.47  −6.52  8150  A0Ia  α Cyg variable,  V450 Car    V450  53921  34000      5.50  −0.35  482  B9IV   53 Per variable ,  HD 92664    V364  92664  52221      5.51  −0.26  466  B9p Si  α2 CVn variable,  HD 67364      67364  39566      5.52  0.11  393  K3/K4III  HD 79698      79698  45219      5.54  −0.28  475  G6II  HD 85656      85656  48310      5.56  −1.78  959  K1IIICN...  HD 64067      64067  38152      5.57  −1.72  934  G5II  HD 46569      46569  31079      5.58  2.73  121  F8V  HD 96706      96706  54327      5.58  −2.12  1128  B2V  variable star,  HD 65907      65907  38908      5.59  4.54  53  G2V...  HD 76113      76113  43499      5.59  −1.12  716  B8III  V448 Car  O  V448  49877  32531      5.60  −0.72  598  K5III  semiregular variable HD 65273      65273  38656      5.62  0.51  343  K3/K4III  HD 68434      68434  39957      5.66  0.33  380  A3m...  HD 89715      89715  50520      5.66  0.90  292  A1V  V372 Car    V372  64722  38438      5.69  −2.56  1462  B1.5IV  β Cep variable,  HD 88661    QY  88661  49934      5.70  −2.29  1294  B2IVnpe  γ Cas variable,  S Car    S  88366  49751      5.71    1780  K5-M6e  Mira variable,  HD 97670      97670  54829      5.73  −3.00  1821  B1.5V  suspected variable HD 65662      65662  38783      5.74  −2.17  1244  K4II  in NGC 2516 HD 93163      93163  52487      5.75  −1.71  1009  B3:V  suspected eclipsing binary,  HD 66194    V374  66194  38994      5.77  −1.72  1028  B2IVnpe  in NGC 2516; γ Cas variable,  HD 81830      81830  46225      5.77  1.47  236  A4V+...  HD 64185      64185  38160      5.78  3.06  114  F1V  spectroscopic binary HD 76538      76538  43669      5.78  −2.35  1376  B5III  HD 85655      85655  48339      5.79  −1.01  746  K2IIICNp...  HD 77615      77615  44256      5.80  −2.13  1259  G8II  HD 84152      84152  47498      5.80  0.57  362  K0/K1III  HD 88473      88473  49764      5.80  −0.46  583  A0IV  HD 49517      49517  32402      5.81  −2.32  1376  K3III  HD 93943      93943  52922      5.85  −1.24  853  B9.5IV/V  HD 80950      80950  45585      5.86  1.32  264  A0V  HD 60060      60060  36444      5.87  0.84  330  K0III  HD 66441      66441  39184      5.87  −0.79  700  B5Vn  suspected variable V482 Car    V482  82536  46620      5.88  −1.68  1058  M2III  semiregular variable V514 Car    V514  92287  52043      5.89  −2.08  1278  B3IV  rotating ellipsoidal variable,  HD 82406      82406  46460      5.90  1.33  268  A0V  HD 82347      82347  46482      5.91  0.06  482  K1III  HD 87283      87283  49164      5.93  −4.03  3196  A9IV  possibly in NGC 3114 HD 90454      90454  50993      5.93  1.13  297  F2III  T Car    T  94776  53394      5.93  1.07  306  K0III  not variable HD 60228      60228  36496      5.95  0.33  433  M1III  HD 94683      94683  53334      5.95  −2.59  1663  K4III  suspected variable HD 54732      54732  34349      5.96  −0.23  564  K0III  HD 56705      56705  35084      5.96  0.58  389  K0V  HD 70839      70839  40932      5.96  −3.36  2380  B1.5III  HD 92436      92436  52127      5.96  −0.53  648  M1III  HD 91533      91533  51623      5.98  −6.71  11241  A2Iab  suspected variable V522 Car    V522  93737  52827      5.98      A0Ia  α Cyg variable HD 81613      81613  46101      5.99  0.92  337  K0III  HD 94650      94650  53272      5.99  −0.89  776  B6V  HD 98560      98560  55280      5.99  3.12  122  F6IV  HD 90874      90874  51194      6.00  1.76  229  A2V  HD 53349      53349  33800      6.01  2.36  175  F0V  suspected variable HD 76346      76346  43620      6.02  1.23  296  A0V  has a planet (b) HD 80094      80094  45418      6.02  0.00  522  B7IV  variable star,  HD 56239      56239  34780      6.03  −0.29  598  A0IV/V  HD 57852      57852  35564      6.05    113  F5V  component of the HIP 35564 system; suspected variable HD 82068      82068  46328      6.05  1.88  223  A3Vn  V390 Car    V390  61966  37248      6.06  −0.05  544  B9IV-Vp...  α2 CVn variable,  V535 Car    V535  98292  55140      6.06  −2.52  1698  M2III  slow irregular variable HD 88825      88825  50044      6.07  −2.84  1976  B4Ve  HD 96544      96544  54294      6.07  −1.81  1226  K2II/III  HD 92682      92682  52150      6.08  −1.57  1105  K3II  variable star,  HD 63382      63382  37854      6.10  −1.20  942  F0II  R Car    R  82901  46806      6.10    416  M6.5 IIIpev  Mira variable,  HD 91619    V369  91619  51676      6.11  −6.99  13583  B7Ia  α Cyg variable,  U Car    U  95109  53589      6.11      G3Ia  classical Cepheid,  HD 70982      70982  40926      6.11  0.34  464  G6/G8III  V461 Car    V461   66546  39225      6.12  −1.92  1320  B2IV-V  Algol variable HD 65908      65908  38863      6.14  0.37  464  B8V  V478 Car    V478  80710  45615      6.14  −1.96  1358  K2III  semiregular variable HD 87543      87543  49281      6.14  −2.49  1734  B4:Vne  HD 95208      95208  53546      6.16  −3.12  2345  K1II  HD 95324      95324  53701      6.16  0.93  363  B8IV  HD 96088      96088  54082      6.16  −3.63  2964  B3III  HD 47001      47001  31265      6.18  −0.17  607  G8III  V492 Car    V492  86659  48782      6.18  −1.43  1087  B3V  53 Per variable HD 87436      87436  49233      6.18  −3.80  3228  A6II/III  suspected variable HD 90630      90630  50976      6.18  0.53  441  A2/A3V  suspected variable V655 Car    V655  91272  51425      6.19  −1.70  1235  B4IV  Algol variable,  HD 62897      62897  37599      6.20  −0.23  629  K0III  HD 75086      75086  42936      6.20  −1.23  997  B7III  HD 87238      87238  49160      6.20  −0.62  753  K1II  HD 84850      84850  47913      6.22  1.68  264  F5IV  HD 89263      89263  50287      6.22  1.63  270  A5V  V532 Car    V532  97451  54708      6.24  −0.53  736  M4III  semiregular variable HD 91767      91767  51732      6.25  −0.78  830  K2/K3III  suspected variable HD 65750    V341  65750  38834      6.25    967  M0III  semiregular variable,  HD 93344      93344  52520      6.25  1.12  346  A5IV/V  HD 52603      52603  33588      6.26  1.59  280  K2III  HD 74622      74622  42717      6.26  1.23  331  K2III  υ Car B  υ    85124        6.26    1623  A8 Ib  component of the υ Car system HD 93372      93372  52535      6.26  3.74  104  F6V  HD 93502      93502  52679      6.26  1.01  365  A0IV  HD 94491      94491  53231      6.26  −2.16  1575  B5V  HD 82858      82858  46737      6.27  −0.40  703  K1III  HD 66607      66607  39238      6.28  −0.28  668  B4V  V375 Car    V375  67536  39530      6.29    1249  B2.5Vn  β Cep variable,  HD 61031      61031  36856      6.29  −1.76  1331  A1III/IV  HD 93662      93662  52797      6.29  −3.35  2763  M1II  suspected variable,  HD 94275      94275  53100      6.29  −0.05  604  A6III  HD 63926      63926  38087      6.30  −2.91  2264  K0III+...  HD 66341      66341  39073      6.30  −1.81  1364  B8III  in NGC 2516 HD 81502      81502  46049      6.30  −2.91  2264  K1/K2II/III  HD 86606      86606  48715      6.30  −2.69  2050  B1Ib  HD 68423      68423  39843      6.32  −0.58  782  B6V  suspected variable HD 80126      80126  45437      6.32  −1.32  1098  G8II  QZ Car    QZ  93206  52526      6.32  −3.23  2650  B0Ib:  in Collinder 228; β Lyr variable,  HD 82458      82458  46407      6.33  2.57  184  F3/F5V  V486 Car    V486  84416  47591      6.33  0.04  592  A0V  β Lyr variable HD 92536      92536  52160      6.33  0.49  479  B8V  in IC 2602 HD 74341      74341  42579      6.34  2.13  227  A3V  HD 90074      90074  50785      6.34  1.23  343  G6III  HD 90289      90289  50916      6.34  −0.59  793  K5Ib-II  suspected variable,  HD 93649      93649  52730      6.34  −2.04  1545  A2IV  HD 97472      97472  54673      6.34  0.08  583  K2/K3III  HD 74148      74148  42440      6.35  0.71  437  A0V  HD 89805      89805  50562      6.35  −2.59  2000  K2II  WR 22    V429  92740  52308      6.35  −4.72  5344  WN7 + A(SB1)  Wolf–Rayet star and Algol variable, ; one of the most luminous stars known HD 93739      93739  52785      6.35  −1.57  1249  B2IV  HD 65189      65189  38667      6.36  −1.08  1003  B8III  HD 72322      72322  41653      6.36  −0.36  721  G0V  V473 Car   V473  76640  43763      6.36  −0.77  869  B5V  53 Per variable HD 79699      79699  45214      6.36  0.21  553  B9V  HD 78632      78632  44665      6.37  0.08  590  K3III  HD 61394      61394  36977      6.39  0.06  601  K1/K2IIICN.  HD 96568      96568  54289      6.39  0.58  473  A3V  HD 44267      44267  29913      6.40  −0.70  858  K2/K3III  variable star,  HD 62758      62758  37530      6.40  −1.18  1069  B2.5V  V368 Car    V368  88647  49926      6.40    801  M3III  semiregular variable,  HD 51210      51210  33012      6.41  0.62  470  A3m...  HD 87438      87438  49223      6.41  −3.23  2763  K3Ib  irregular variable,  HD 91270      91270  51461      6.41  −0.57  811  M2III  suspected variable HD 84046      84046  47422      6.42  0.01  623  B8/B9III/IVw...  suspected variable,  HD 88907      88907  50067      6.42  −1.06  1022  B2V  V507 Car    V507  90966  51265      6.42  −2.56  2037  B2/B3III:ne  Be star HD 91094      91094  51327      6.42  0.00  627  M1III  semiregular variable HD 98025      98025  55003      6.42  0.16  583  A3V  HD 78293      78293  44565      6.43  −1.21  1101  A8III  HD 93359      93359  52537      6.43  1.25  354  A6IV  HD 65867      65867  38963      6.44  0.43  518  A8/A9IV  suspected eclipsing binary V469 Car    V469  72303  41644      6.44  −0.28  720  Ap Si  α2 CVn variable HD 49705      49705  32477      6.45  0.93  414  G6III  HD 81896      81896  46143      6.45  0.06  617  K1III  V495 Car    V495  88158  49642      6.45  −0.55  817  Ap Si α2 CVn variable WR 24      93131  52488      6.46  −5.05  6520  WN7 + A  in Collinder 228; Wolf–Rayet star, ; one of the most luminous stars known HD 52622      52622  33577      6.46  1.46  326  F2II  suspected variable HD 54967      54967  34350      6.46  −1.79  1455  B3V  HD 93738      93738  52815      6.46  0.67  469  B9.5V  in IC 2602 HD 49219      49219  32269      6.47  −0.30  736  B5/B6V  variable star,  HD 70267      70267  40655      6.47  2.01  254  F5V  V487 Car    V487  84809  47893      6.47  −0.66  869  B8III/IV  α2 CVn variable HD 93695      93695  52806      6.47  −1.41  1230  B5Vvar  HD 95122      95122  53556      6.48  −0.55  832  B7V  suspected variable HD 92399      92399  52103      6.50  −1.82  1502  B4/B5III/IV  HD 96248    V414  96248  54179      6.58    3700  B1Iab  α Cyg variable,  HD 57853      57853  35564      6.63    113  F9V  component of the HIP 35564 system QX Car    QX  86118  48589      6.64    1610  B2V  Algol variable,  HD 96446    V430  96446  54266      6.68    1540  B2k  β Cep variable,  HD 53143      53143  33690      6.68    59.74  G9V  has a circumstellar disk VY Car    VY  93203  52538      6.91    9100  F7Iab/Ib  classical Cepheid,  AG Car    AG  94910  53461      6.96    17000  B2-3Ib/WN11  luminous blue variable,  BO Car    BO  93420        7.18      M4Iab:  semiregular variable,  HD 93403      93403  52628      7.30    2670  O5.5I+O7V  binary star HD 93129A      93129A        7.31    7500  O2If*+O3.5  in Trumpler 14; binary star; primary is one of the most luminous stars known V Car    V  72275  41588      7.31    5600  G2Iab:  classical Cepheid,  HD 93843      93843        7.33      O5III(f)v  irregular variable,  HD 95086      95086  53524      7.36    295  A8III  has a planet (b) HD 93250      93250  52558      7.50    7500  O4IIIfc  in Trumpler 16; suspected variable HR Car    HR  90177  50843      7.57    17700  B3Iaep  luminous blue variable,  WR 40    V385  96548  54283      7.70    5900  WN8h  Wolf–Rayet star and rotating ellipsoidal variable, ; one of the most luminous stars known HD 93205    V560  93205        7.75    7500  O3.5V((f+))  in Trumpler 16; rotating ellipsoidal variable,  IW Car    IW  8208482085        7.90      A4Iab/II:  RV Tau variable,  HD 65216      65216  38558        7.98    112  G5V  has two planets (b & c) HD 97152    V431  97152  54574      8.07    4000  WC7+O7V  Wolf–Rayet star; eclipsing binary,  HD 63765      63765  38041      8.10  5.53  106  G9V  Tapecue; has a planet (b) Y Car    Y  91565  51653      8.16    3050  F2  double-mode Cepheid,  HD 51608      51608  33229      8.17    114  K0IV  has two planets (b & c) HD 85628 A      85628         8.19    559  A3V  has a planet (b) YZ Car    YZ  90912  51262      8.24    5900  G5  classical Cepheid,  WR 16    V396  86161  48617      8.32      WN8h  rotating ellipsoidal variable, ; one of the most luminous stars known EM Car    EM  97484        8.52      O8V  Algol variable RT Car    RT  303310  52562      8.55    1430  M2Iab:  possibly in Trumpler 15; irregular variable, , one of the largest stars known HD 85567    V596  85567  48269      8.57    6900  B2  FS CMa variable,  UX Car    UX  91039  51338      8.62    2530  F2II  classical Cepheid,  XZ Car    XZ  305996  54101      8.67      B2:pe  classical Cepheid,  GG Car    GG  94878  53444      8.70      B0/2eq  Be star and re-radiating binary system,  V403 Car    V403          8.74    8400  B1III  in NGC 3293; β Cep variable,  Tr 16-104    V572          8.75    7500  O7V((f))+O9.5V+B0.2IV  in Trumpler 16; Algol variable,  V348 Car    V348  90707        8.78      B1III  β Lyr variable,  WR 25    V396  93162        8.80    7500  O2.5If*/WN6  in Trumpler 16; Wolf–Rayet star; one of the most luminous stars known HD 60435    V409  60435  36537      8.89    739  Ap...  rapidly oscillating Ap star WR 23      92809  52331      9.03    3400  WC6  Wolf–Rayet star HD 92024    V381  92024        9.04    8400  B1III  in NGC 3293; β Cep variable,  GH Car    GH  306077  54621      9.20      G0  classical Cepheid,  WZ Car    WZ  94777  53397      9.37    4700  F8  classical Cepheid,  CPD -59° 2635    V731          9.43    7500  O8V+O9.5V  in Trumpler 16; Algol variable,  V392 Car    V392          9.49      A2Vp...  in NGC 2516; Algol and α2 CVn variable,  XY Car    XY  308149  53945      9.49      G5  classical Cepheid,  HD 87643    V640  87643        9.50      B2e  Orion variable,  CPD -59 2628    V573          9.52    7500  O9.5V+B0.3V  in Trumpler 16; Algol variable HD 90657    V398  90657  51109      9.69    3500  WN5+O4-6  Wolf–Rayet star; eclipsing binary,  GL Car    GL  306168        9.70      B3:V  Algol variable DW Car    DW  305543        9.85      B2:pe  in Collinder 228; Algol variable SS73 17    V648          9.99      M3pe+OB   Z And variable ,  CPD -57 2874              10.16      sgB1[e]  B[e] star GZ Car    GZ  302719  50615      10.20    2400  G5  double-mode Cepheid,  HH Car    HH  303503        10.31      B  Algol variable,  EY Car    EY    52380      10.35      B2:pe  double-mode Cepheid,  HD 307938    V557  307938        10.57      G2V  BY Dra variable,  WR 18    V500  89358  50368      10.6    6300  WN4-s  Wolf–Rayet star HD 94546    V428  94546  53274      10.7      WN4+O8V  Wolf–Rayet star; eclipsing binary,   He 3-519               10.85      WN11  Wolf–Rayet star,  NGC 3603-A1      97950A        11.12    20000  WN6ha+O3V  in NGC 3603; Algol variable,  both components among the most luminous and massive stars known CR Car    CR          11.30      B2:pe  classical Cepheid,  NGC 3603-B      97950B        11.33      WN6h+abs  one of the most luminous and most massive stars known Innes' star              11.52    41.31  M3.5  has a planet QU Car    QU  310376  54226      11.54    1290  B+...   V Sge variable ,  WR 30    V541  94305        11.73      WC6+O7.5V  Algol variable,  WRA 751    V432          11.79      WR:  luminous blue variable,  NGC 3603-C      97950C        11.89      WN6h+abs  spectroscopic binary FO 15    V662          12.09    7500  O5.5V+O9.5V  in Trumpler 16; Algol variable,  Sher 25              12.27      B1.5Iab  in NGC 3603; potential supernova progenitor WR 30a    V574          12.73      WR+...  Algol variable,  GJ 1128              12.78      M4.0V  He 2-38    V366          12.92      M5-7.5  Mira and Z And variable,  BPM 6502    V727          13.09      DA2.2+M  re-radiating binary system WR 20a    V712          13.5      O3If*/WN6+O3If*/WN6  in Westerlund 2; Algol variable LHS 288              13.92    15.602  M4   OGLE-TR-113    V752              14.42    1800  K  has a transiting planet (b) 2S 0921-630    V395          15.3      K0IIIe  low-mass X-ray binary OGLE-TR-123    V816            15.47      FV+MV  possibly has a transiting planet OGLE-TR-111    V759            15.55    5000  G  has a transiting planet (b) anda possible second planet OGLE-TR-132    V742            15.72    7110  F  has a transiting planet (b) OY Car    OY          16.2    277  M5/M6:...   SU UMa variable  and eclipsing binary,  OGLE-TR-182              16.84    12700  G  has a transiting planet (b) OGLE-TR-211                  5300  F  has a transiting planet (b) OGLE-TR-122    V817                    has a transiting brown dwarf OGLE2-TR-L9                  2935  F3  has a transiting planet (b) 1E 1048.1-5937                    Be  anomalous X-ray pulsar DENIS J081730.0-615520                  16.1  T6  brown dwarf PSR J1048-5832                        pulsar PSR J1119-6127                        pulsar

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