Table 3
Optical Properties of Candidate Young Stellar Objects with Echelle Spectra

Object^a
	R.A.(2000)	Decl.(2000)	Date	Sp. Ty. Range	Sp. Ty.^b
	Surface	v sini
^c
	YSO?^d
	
	(hh mm ss.s)	(



 

'")	(YYMMDD)			Gravity	(km s



 

)		
SCB 40	18:28:56.2	01:06:27.6	2009 Aug 11	F7-G0	G0	V-IV	16 +or- 2 - 25 +or- 2	 ... 	
SCB 41	18:28:58.4	01:10:59.7	2009 Aug 11	A9-F2	F4	cdots	34 +or- 8	 ... 	
SCB 43	18:29:08.0	01:05:25.4	2009 Aug 11	F6-F9	F7	V-III	cdots	 ... 	
WMW 124	18:29:08.2	01:05:43.1	2009 Jun 09	A1-A3	A1	V-III	40 +or- 12	IRX, TD	
 ... 	 ... 	 ... 	2010 Jul 10	 ... 	 ... 	 ... 	 ... 	 ... 	
BD+01 3686	18:29:27.6	01:12:56.8	2009 Aug 11	F2-F6	F6	V-III	24 +or- 4	X	
BD+01 3687	18:29:31.7	01:08:19.1	2009 Jun 09	F3-F9	F6	V-IV	16 +or- 3	ref. neb.	
 ... 	 ... 	 ... 	2010 Jul 10	 ... 	 ... 	 ... 	 ... 	 ... 	
WMW 82/KOB 173	18:29:33.4	01:08:22.8	2009 Jun 09	A3-A4	A3.5	V	cdots	IRX, ref. neb.	





 

/XMM	18:29:56.1	01:00:21.7	2010 Jul 10	B3-B6	B6	III	cdots	X, ref	
WMW 193/BD+01 3689B	18:29:57.5	01:10:46.4	2010 Jul 10	A1-A8	A5	V-III	140 +or- 16	X	
WMW 192/HD 170545	18:29:57.6	01:10:52.9	2010 Jul 10	A1-A3	A2.5	V	31 +or- 4	X	
 ... 	18:30:07.4	01:01:01.5	2009 Aug 11	G6-K2	G9	IV	cdots	 ... 	
KOB 370	18:30:08.7	00:58:46.5	2010 Jul 11	G9-K4	K1	IV	cdots	Li,Halpha,IRX^e
	
BD+1 3693	18:30:10.4	01:19:33.7	2009 Aug 11	A5-A8	A7	III	cdots	 ... 	
WMW 220	18:30:24.5	01:19:50.7	2009 Aug 11	K0-K2	K1	cdots	14 +or- 1	X	
HD 170634	18:30:24.9	01:13:23.0	2010 Jul 10	B6-B9	B9	III	cdots	ref. neb.	
XMM	18:30:37.4	01:17:58.3	2010 Jul11	F8-K5	K0	V-IV	41 +or- 3	X	
 ... 	18:30:42.3	00:58:48.9	2010 Jul 11	F4-F6	F5	III	42 +or- 3	 ... 	
SCB 70	18:30:54.5	01:12:52.7	2009 Aug 11	F4-F7	F7	V-IV	16 +or- 2 - 24 +or- 2		

a Source names from X-ray, optical or infrared studies by: (SCB) Straizbreveys et al. (1996), (XMM) XMM-Newton survey by Preibisch (2003), (WMW) Spitzer survey by Winston et al. (2007), (CDF88) reflection nebulae survey by Chavarria-K. et al. (1988) , (KOB) ISO survey by Kaas et al. (2004).
b Spectral types derived from Magellan spectra only; See Table 4 for adopted spectral type.
c In most cases, the value of v sin i was not sensitive to surface gravity and is represented by a single value. A range is given only for SCB 40 and SCB 70. When the surface gravity was indeterminate, a dwarf surface gravity was assumed. Errors are the standard deviation of the mean.
d YSO criteria include an infrared excess (IRX) including transition disk objects (TD), X-ray emission (X), association with reflection nebulosity (ref. neb.), Halpha emission with EW >10 angst (Halpha), or lithium absorption (Li).
e Halpha emission is variable and not detected in the echelle spectrum.