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Table 2:

Studied stars, SFRs positionally coincident and summary of the observations.
  $\alpha $ (J2000.0) $\delta$ (J2000.0) l b   $d_{\rm SFR}$ $t_{\rm exp}$   Date(s)
Stara [ h  m    s  ] [ $^\circ$   '    ''  ] [deg] [deg] SFR [pc] [s] S/Nb [yyyy-mm-dd]
CD-38 4380 08 23 11.86 -39 07 01.5 257.32 -1.06 Gum Nebula 200-240 1200 25 2004-04-03
WRAY 15-488 10 01 48.11 -59 12 12.5 282.70 -3.17 ScoOB2-5 145  800 25 2004-04-04
WRAY 15-522 10 12 12.42 -62 32 33.1 285.69 -5.13 ScoOB2-5 145 1500 25 2004-04-05
Th 35-41 10 25 40.07 -58 22 17.4 284.78 -0.73 ScoOB2-5 145 1800 15 2004-04-08
Hen 3-416 10 25 44.51 -58 33 52.2 284.89 -0.89 ScoOB2-5 145 1200 30 2004-04-07
WRAY 15-566 10 25 51.36 -60 53 13.2 286.13 -2.86 Low.Cen.Crux - ScoOB2-5 118-145 1800 10 2004-04-07
HD 305773 10 56 03.88 -60 29 37.6 289.18 -0.74 Low.Cen.Crux - ScoOB2-5 118-145  700 100 2008-05-21
WRAY 15-770 11 11 28.49 -63 00 23.7 291.87 -2.30 Low.Cen.Crux - ScoOB2-5 118-145 1200 10 2004-04-05
Hen 2-80 12 22 23.18 -63 17 16.8 299.67 -0.60 Low.Cen.Crux - ScoOB2-4 118-145 1800 25 2004-04-08
Hen 3-823 12 48 42.39 -59 54 35.0 302.59 2.96 Low.Cen.Crux - ScoOB2-4 118-145  900 60 2008-04-21
Th 17-35 13 20 03.59 -62 23 54.0 306.24 0.29 Low.Cen.Crux - ScoOB2-4 118-145 1800 25 2004-04-08
WRAY 15-1104 13 29 51.02 -56 06 53.7 308.30 6.36 Low.Cen.Crux - ScoOB2-4 118-145 1500 40 2004-04-06
WRAY 15-1372 15 53 50.59 -51 43 05.1 329.21 1.59 Up.Cen.Lup 140 1500 30 2004-04-08
Hen 3-1121N 15 58 09.62 -53 51 18.3 328.345 -0.463 ... - 1500 70 2008-04-21
Hen 3-1121S 15 58 09.67 -53 51 34.9 328.342 -0.466 ... - 1500 85 2008-04-24
Hen 3-1145 16 08 54.69 -39 37 43.1 339.21 8.95 Up.Cen.Lup 140 2000 16 2004-04-08
WRAY 15-1435 16 13 06.68 -50 23 20.0 332.36 0.58 ... - 1800 55 2008-04-24
HD 145718 16 13 11.59 -22 29 06.6 352.43 20.44 $\rho$Oph - Sco OB2 110 - 160 1000 20 2004-04-08
HD 152291 16 54 24.20 -40 39 09.0 344.40 1.88 Up.Cen.Lup 140  600 100 2008-04-21
Hen 3-1347 17 10 24.15 -18 49 00.7    4.10 12.26 ... - 1800 70 2007-08-04
WRAY 15-1651 17 14 45.03 -36 18 38.4 350.27 1.35 ... - 2400 17 2008-05-01
WRAY 15-1650 17 15 32.79 -55 54 22.7 334.28 -10.07 ... - 900 8 2007-08-17
HD 323154 17 23 02.36 -39 03 52.5 348.96 -1.57 ... - 600 120 2007-08-04
WRAY 15-1702 17 24 30.88 -37 34 27.7 350.35 -0.97 ... - 1700 8 2008-04-30
MWC 878 17 24 44.70 -38 43 51.4 349.42 -1.65 ... - 900 70 2007-08-04
AS 231 17 30 21.66 -33 45 29.6 354.18 0.17 ... - 1400 140 2004-07-31
Hen 3-1428 17 35 02.49 -49 26 26.4 341.41  -9.03 ... - 1200 50 2007-08-07
HD 320156 17 37 58.51 -35 23 04.3 353.66 -2.03 ... - 600 90 2007-08-07
MWC 593 17 49 10.16 -24 14 21.2    4.43   1.75 ... - 720 85 2007-07-31
HD 313571 18 01 07.18 -22 15 04.0    7.53   0.39 ... - 900 70 2007-08-02
MWC 930 18 26 25.24 -07 13 17.8  23.65   2.23 ... - 2100 50 2007-08-04
MWC 953 18 43 28.43 -03 46 16.9  28.69   0.05 ... - 1200 60 2007-07-31
AS 321 18 47 04.80 -11 41 02.3  22.02  -4.35 ... - 1500 75 2004-07-31
MWC 314 19 21 33.97 +14 52 57.0  49.57   0.25 ... - 900 65 2007-08-04

Notes. (a) All sources from Table 4b of Thé et al. (1994), except for Hen 3-1145 (Table 2), Hen 2-80 (Table 4a) and CD-38 4380 and HD 145718 (Vieira et al. 2003).
(b) The S/N is the average S/N in the continuum close to the H$\alpha $ line.


Source LaTeX | All tables | In the text

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