Table 4: The final 11 O-type field stars that could not be associated with clusters. An asterisk indicates if the surrounding field shows signs of star formation as reported in Paper I. The abbreviations are the same as in Tables 1 and 2.
Name VM SM

HD 39680 OPT C

HD 48279^* OPT C

HD 96917 single SB1:

HD 112244 VB SB1:

HD 120678 single U

HD 123056^* single C

HD 124314^* VB SB1:

HD 154811 single C

HD 165319^* single C

HD 193793 VB SB2O

HD 202124 single C

**Table 4:** The final 11 O-type field stars that could not be associated with clusters. An asterisk indicates if the surrounding field shows signs of star formation as reported in Paper I. The abbreviations are the same as in Tables 1 and 2.
Name	VM	SM
HD 39680	OPT	C
HD 48279^*	OPT	C
HD 96917	single	SB1:
HD 112244	VB	SB1:
HD 120678	single	U
HD 123056^*	single	C
HD 124314^*	VB	SB1:
HD 154811	single	C
HD 165319^*	single	C
HD 193793	VB	SB2O
HD 202124	single	C

Source LaTeX | All tables | In the text

	1 Introduction
	2 Main results from Paper I
	3 The field O stars as candidate runaway stars
	4 Discussion
	5 Conclusion
	Appendix A: Clusters near HD 52533 and HD 195592
	References