N-body simulations in reconstruction of the kinematics of young stars in the Galaxy

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Table 1:

Observed residual velocities of OB-associations in the stellar-gas complexes.
Region	R	$V_{R~{\rm obs}}$	$V_{\theta~{\rm obs}}$	l	r	Associations
	kpc	km s^-1	km s^-1	deg.	kpc

Sagittarius	5.6	$+9.9\pm2.4$	$-1.0\pm1.9$	8-23	1.3-1.9	Sgr OB1, OB7, OB4, Ser OB1, OB2,
						Sct OB2, OB3;
Carina	6.5	$-5.8\pm3.3$	$+4.7\pm2.2$	286-315	1.5-2.1	Car OB1, OB2, Cru OB1, Cen OB1,
						Coll 228, Tr 16, Hogg 16, NGC 3766, 5606;
Cygnus	6.9	$-5.0\pm2.6$	$-10.4\pm1.4$	73-78	1.0-1.8	Cyg OB1, OB3, OB8, OB9;
Local System	7.4	$+5.3\pm2.8$	$+0.6\pm2.5$	0-360	0.1-0.6	Per OB2, Mon OB1, Ori OB1, Vela OB2,
						Coll 121, 140, Sco OB2;
Perseus	8.4	$-6.7\pm3.0$	$-5.9\pm1.5$	104-135	1.8-2.8	Per OB1, NGC 457, Cas OB8, OB7, OB6,
						OB5, OB4, OB2, OB1, Cep OB1;

Source LaTeX | All tables | In the text

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