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from catalogue J/ApJS/112/109.
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## (from tabmap V6.0 (2016-08-18)) 2024-04-28T19:02:41 #--------------------------------------------------------------------------- #-- J/ApJS/112/109 Rho Oph Near-IR Positions and Photometry (Barsony+, 1997) #-------------------------------------------------------------------------- #---Table: J/ApJS/112/109/./notes.dat Notes for table3.dat (28 records) # Note A1 --- Symbol used in table3 # Text A77 --- Text of note attached to symbol ------------------------------------------------------------------------------- N| o| t| e|Text -|----------------------------------------------------------------------------- *|indicates indicate positional difference: 5-10arcsec for a single asterisk, *|and 10-15arcsec for a double asterisk a|Examination of the POSS plates, object colors, and magnitudes leads to this a|identification, despite the positional disagreement. b|Despite the approx. 1.5 arcsec positional discrepancy, this identification is b|made on the basis of good agreement of object colors and magnitudes. c|GSS 37's published position is 62 arcsec offset from BKLT 162642-242031. d|BBRCG 6 and BBRCG 7 form a binary system unresolved by our survey. e|BBRCG 8 and BBRCG 10 form a binary system unresolved by our survey. f|GSS 40 is a blend of BKLT 162653-242229 and 162654-242231. g|WL 21 and WL 22 are not listed in Wilking & Lada 1983 but are referred to in g|Wilking et al. 1989. h|BKLT 162658-243739E and W both fall within positional and photometric errors h|of CRBR 51 = SKS 3-24. i|Elias 28 is a pair of T-Tauri stars: BKLT 162658-244534 and 162658-244529 i|(Elias 1978). j|VSSG 31 is a blend of BKLT 162704-242830 and 162706-242837. k|VSSG 23 = Elias 30 both encompass the candidate 6[&farcs;]5 separation binary k|pair BKLT 162710-241914 and 162710-241921 l|BKLT 162715-243843 = WL 20 is actually a triple system (M. Ressler 1996, l|private commmunication) previously resolved as a binary. m|VSSG 26 is a blend of these four sources, which include WL 3, WL 4, and WL 5. n|SKS 3-55 is a candidate 3 arcsec separation binary composed of n|BKLT 162731-243752 and 162731-243755. o|VSSG 14 = Elias 36 is a blend of BKLT 162749-242522 and 162749-242540. p|GY 426 = IRS 57 is a 4 arcsec separation binary candidate composed of p|BKLT 162759-242159 and 162759-242202. q|VSSG 15 = Elias 38 is a blend of BKLT 162809-242322 and 162810-242305. -------------------------------------------------------------------------------