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Table 3:

Fitted parameters and derived results using CN&P's spherical model for the expanding shells defined by the H I features surrounding the Sco-Cen association.
Stellar $l_{\rm o}, b_{\rm o}$ $2\theta$ $V_{\rm s}$ n V0 $r_{\rm o}$ R $d_{\rm MIN}$ $d_{\rm MAX}$ $d_{\rm OBS}$ $\tau_{\rm s}$ Fitted H I-features
subgroup ( $\hbox{$^\circ$ }$)   km s-1    km s-1  (pc) (pc) (pc) (pc) (pc)  Myr  
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
UCL 325 $\pm$ 5, 130 +3 1 8 140 127 13 267 <76 15.6 ) A1, A'1, B1,B2, B', B'', C,
  17.5 $\pm$ 5 $\pm$10   2 10           12.7 } LCC-br., M1?, C'?,
        3 12           10.6 ) nearby H I in GQ II at V>0?
US 350 $\pm$ 5, 46 +3 1 10 145 57 88 202 <130 5.7 ) B1, B'', SvW cloud?,
  21 $\pm$ 4 $\pm$6   2 12           4.8 ) US-loop
(US- 346 $\pm$ 5, 28 +3 1b 8 130 31 99 161   1.0 US-loop
loop) 25 $\pm$ 5 $\pm$4   2b 10           0.8 interior of US-loop = substr.
LCC 300 $\pm$ 5, 90 +2 1 6 118 83 35 201 <60 13.8 ) LCC-branch and clump,A2,
  10 $\pm$ 5 $\pm$8   2 9           9.2 } B2,B', M1?, M2?, SvW cl.?,
        3 12           6.9 ) C?, Cha arc = substr.


Source LaTeX | All tables | In the text

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