The interstellar medium surrounding the Scorpius-Centaurus association revisited

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Table 4:

Main molecular dark cloud complexes located within the region studied in this paper. (See the text for the details)
mdcc	$l (\hbox{$^\circ$ })$ ,	$\bar{V}_{\rm LSR}$	$\bar{d}$	$M_{\rm mol}$
	$b (\hbox{$^\circ$ })$	(km s^-1)	(pc)	( $M_\odot$ )
(1)	(2)	(3)	(4)	(5)
Oph¹	350-370,	-1 to +6	140	9000
	+6 to +24		(80-200)
Lup²	335-350,	-4.5 to +10	150 $\pm$ 10	17 000
	+5 to +25
Cha-Mus³	292-316,	+0.5 to +7	150-180	8300
	-33 to -8
Aql Rift⁴	376-394	+5 to +10	200	150 000
	0 to +20
Aql South⁵	386-400	0 to +15	<220	4000
	-25 to -12

References. 1) de Geus et al. (1990); de Geus & Burton (1991); 2) Tachihara et al. (2001); Magnani et al. (1996); Rizzo et al. (1998); 3) Mizuno et al. (2001); 4) Dame et al. (1987, 2001); 5) Kawamura et al. (1999).

Source LaTeX | All tables | In the text

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