HD 3125   The primary should be G7 III-IV.
HD 3210   The near-UV spectrum is almost entirely that of the hot component.
HD 4775   To accord with Hipparcos parallax and the observed {Delta}Mv, the 
HD 4775    primary should be a class II-III giant (Mv=-1.25) and the secondary a
HD 4775    hot giant. However, Mason et al. (1997AJ....114.1607M) do not retain 
HD 4775    this hypothesis, and also our IR spectra indicate more probably a 
HD 4775    normal giant G7 primary than a higher luminous one.
HD 5373   Griffin (1989Obs...109...79G) comments that the mass function of the 
HD 5373    system, f(m)=0.453, is surprisingly large; however, our 
HD 5373    classification is compatible with such a value of f(m) and does not 
HD 5373    require that the secondary be double.
HD 8226   No IR classification; spectral subtraction indicates ~G8 III.
HD 9352   K3 Ib-II is an average of the IR classifications (Ginestet et al.,
HD 9352    1997, Cat. <J/A+AS/123/135>, 1999A&AS..134..473G). 
HD 9352    Secondary is B7 or B8.
HD 11154  Hot component strongly resembles the MK standard HD 11636 (A5 V), 
HD 11154   which, according to its Hipparcos data, should be A5 IV.
HD 13474  B9 according to H lines only, because the primary's K line was 
HD 13474   incompletely subtracted. Weak IS line.
HD 16082  The high value of f(m)=1.52 (Griffin, 1990JApA...11..491G) suggests 
HD 16082   that the secondary is double.
HD 17245  B8, but He is weak: could be B9. IS K line visible.
HD 17479  See HD 13474; subtraction of the primary's K line probably incomplete.
HD 17479   Strong IS K line; secondary is B9.5 or B9 if we adopt color excesses 
HD 17479   of 0.14 and 0.20, respectively.
HD 17718  A0 or B9.5; K line asymmetrical.
HD 17878  The Balmer lines and the K line do not correspond to the same MK type;
HD 17878   the K line, which is unusually broad and shallow, indicates a type 
HD 17878   between A2 and A4 (see text Sect. 2.4).
HD 18715  The composite spectrum is ADS 2286 A; ADS 2286 B (sep. 8") 
HD 18715   is HD 18716, quoted as A7 IV in SIMBAD.
HD 18925  The primary should be G9 II-III.
HD 19091  A0 or A1: the Balmer lines resembles those of the MK standard 
HD 19091   HD 21447, of type A1 V; faint (IS) K line. Probably rapid rotation.
HD 19278  No parallax from Hipparcos. E(B-V) estimated from the strength of the 
HD 19278   IS K line.
HD 19926  Secondary could be double and perhaps Ap; Asymmetrical K line.
HD 20084  The presence of a secondary is suggested only by a strengthening of 
HD 20084   the lines of Sr II 4077 and H{delta}. The precise Hipparcos parallax 
HD 20084   shows that the type F0 V given by Markowitz (1969, Ph.D. thesis, Ohio
HD 20084   State Univ.) is suspect; it cannot be earlier than F5 V.
HD 23089  Supergiant G primary: see Sect. 5.
HD 24480  Poor-quality subtraction; the secondary appears to be near B8-B9.
HD 26630  A weakened K line is the only indication of a composite spectrum. The 
HD 26630   star is an MK standard for G0 Ib (Garcia, 1989, Cat. <III/149>); the 
HD 26630   type of B9.5 V is from Stickland (1988IUE88...2...27S). Supergiant G 
HD 26630   primary: see Sect. 5.
HD 26673  A0 or B9.5, K line is rather square: double?
HD 27395  The large color excess implied by our model conflicts with the 
HD 27395   weak IS K line.
HD 27639  See HD 27395 (same problem). B7 or B8?
HD 29094  Between B8 and B9.5 (poor subtraction). Supergiant G primary: 
HD 29094   see Sect. 5.
HD 29104  Almost certainly Am.
HD 32835  Primary could be CP (possibly Ba star). Secondary between B6 and B8, 
HD 32835   but if B6 or B7 then it must be He-weak. The model indicates a large 
HD 32835   color excess (see Sect. 2.4).
HD 33883  The model implies A5 III, but a double secondary is also a possibility
HD 34318  Model doubtful; the subtracted spectrum does not correspond to an MK 
HD 34318   standard, and the K line has a narrow core with a widened base.
HD 34533  Either A2 with low rotation, or marginal Am.
HD 36947  Supergiant G primary: see Sect. 5.
HD 39118  Double secondary (Griffin, 1990JApA...11..491G); one of the hot stars 
HD 39118   is probably A0.
HD 45044  B9/A0; if the hot star is B9, then the IS K line is too strong for the
HD 45044   color excess of 0.16 mag, as given by the model.
HD 49635  Could be Bp Cr, Sr:
HD 50820  In the near-UV the observed spectrum is almost entirely that of the 
HD 50820   hot star (as for HD 3210). Strength of IS K line appears to disagree 
HD 50820   with E(B-V)=0.44; however, {epsilon}{pi}/{pi}=1.17.
HD 51424  Could be a marginal Am.
HD 52690  Very poor subtraction; B7 to B9.
HD 52822  Resembles the MK standards HD 123299 (A0 III) and HD 23873 (B9.5 V).
HD 55684  Negative parallax!
HD 59067  Rapid rotation; spectral type near B2. Supergiant G primary: 
HD 59067   see Sect. 5.
HD 59604  Am (A4, A5, F0 for the K line, the hydrogen line, and the metallic 
HD 59604   lines, respectively).
HD 63023  The subtracted spectrum corresponds to that of the MK standard 
HD 63023   HD 123299 (A0 III).
HD 70442  Between A0 and A2. Classification difficult: on one of our spectra the
HD 70442   K line is double (double secondary or K-line emission?), IS K-line 
HD 70442   would be surprising since the distance is only 138 pc.
HD 70826  Secondary seems to be a double-lined Am; low rotation, K line ~A2, 
HD 70826   H lines ~A3. However, a model with a double secondary is too luminous
HD 70826   in relation to the Hipparcos data. We have therefore included another
HD 70826   model with a single secondary A3 V, which agrees with the 
HD 70826   Hipparcos Mv.
HD 73451  Difficult to judge between B9.5 and AO. The model could equally well 
HD 73451   have B9.5 IV. Possibly Bp or Ap, because Sr II seems enhanced.
HD 74228  Secondary dominant in the UV (see Sect. 4.3.2).
HD 74395  The only hint of compositeness is a weakening of the cool star's K 
HD 74395   line; the subtraction, although was difficult, have been carried out.
HD 74395   Supergiant G primary: see Sect. 5.
HD 83808  The model slightly differs to the one given in a previous paper 
HD 83808   (Hummel et al., 2001AJ....121.1623H). The primary is also a CP star 
HD 83808   (Griffin, 2002AJ....123..988G).
HD 84367  Secondary should be Am but the model indicates class III; therefore 
HD 84367   possibly of type {delta} Del. The Hipparcos {Delta}m (0.9) value 
HD 84367   disagree with our spectroscopic estimation (~-0.2); Heintz 
HD 84367   (1982A&AS...47..569H) gives a visual orbit with {Delta}m=0, he notes 
HD 84367   also that the components fit luminosity class III.
HD 102509 Asymmetrical K line, perhaps because the system is a (known) 
HD 102509  RS CVn-type binary.
HD 126269 Secondary spectrum strongly resembles the MK standard HD 97633 (A2V),
HD 126269  but on the basis of its precise parallax its Mv is that of a giant. 
HD 126269  Very low rotation; marginal Am?
HD 137975 Possible that the primary is CP (Ba?); poor-quality subtraction.
HD 139137 Could be Am.
HD 157978 Could be B9.5 V. Double K line, triple spectroscopic system 
HD 157978  (Batten, Fletcher, & McCarthy, 1989, Cat. <V/64>).
HD 159870 The primary could be a Ba star: see Sect. 7). 
HD 159870  Secondary is Am ({delta} Del?); the K line indicates A6/7.
HD 164252 Double system (sep. 19.6"); spectra obtained separately. Hipparcos 
HD 164252  data refer to the G7 II-III primary. Secondary is HIP 88051.
HD 166479 Possibly A0. The K line has a weak blend in its redward wing.
HD 167570 Poor-quality spectra, and unreliable subtraction. Secondary could be 
HD 167570  A4, but that would imply E(B-V)=0.28 although the distance is 
HD 167570  only 186pc. The Balmer lines indicate a later type. The composite 
HD 167570  spectrum strongly resembles that of HD 17878.
HD 168701 Between B3 and B5; poor-quality spectra and unreliable subtraction.
HD 169689 Si lines rather strong; possibly B9p Si?
HD 169985 Double K line. Triple spectroscopic system 
HD 169985  (Batten et al., 1989, Cat. <V/64>).
HD 174016 Secondary is A0p Sr Cr Eu Si (Ginestet et al., 1999A&AS..140..279G).
HD 183912 B8p Si Cr Eu: Sr:; a small IS K line surprising, since d=118pc.
HD 184398 Strong Ca II emission in the primary (K2 II-IIIe). Secondary has a 
HD 184398  shell spectrum. Subtraction difficult, so type A1 is uncertain.
HD 186097 Supergiant G primary: see Sect. 5.
HD 186203 Supergiant G primary: see Sect. 5.
HD 187299 No UV spectrum observed; Griffin & Griffin (1979MNRAS.187...91G) 
HD 187299  gives ~B7 for the secondary. Bersier (1996A&A...308..514B) 
HD 187299  gives E(B-V)=0.57.
HD 187321 Supergiant G primary: see Sect. 5. Negative parallax!
HD 190361 No UV spectrum observed; secondary type B4 IV-V from 
HD 190361  Griffin & Griffin (1997MNRAS.285..472G).
HD 192577 Between B2 and B4; He lines very strong.
HD 192644 No UV spectrum observed. Griffin (2001Obs...121...91G) suggests A2 V.
HD 192713 Between B7 and B9 (poor subtraction). Supergiant G primary: 
HD 192713  see Sect. 5. Our model is similar to that of 
HD 192713  Griffin et al. (1993A&A...274..225G).
HD 192909 Between B4 and B5 (poor subtraction). Strong Ca II emission from the 
HD 192909  primary.
HD 193410 Possibly Bp Sr.
HD 193469 No trace of the secondary in the near-UV. Type B8 from 
HD 193469  Stickland (1988IUE88...2...27S).
HD 193495 Possibly B9p Si. Ca II K (interstellar?) is present, although d=105pc 
HD 193495  (see HD 183912).
HD 196088 B9, but also close resemblance to HD 123299 (MK standard A0 III).
HD 196093 Secondary appears to be He rich.
HD 197177 MK standard G8 IIb. Visual double (sep. ~3"); our UV spectrum is that
HD 197177  of the primary. Secondary type of A0 from 
HD 197177  Parsons & Ake (1998, Cat. <J/ApJS/119/83>).
HD 198810 Very similar to MK standard A7 V (HD 6961); low rotation; 
HD 198810  possibly marginal Am.
HD 199378  Poor-quality subtraction.
HD 200428 No UV spectrum observed; secondary type of A5 from Henry Draper's 
HD 200428  catalog, and retained by Griffin et al. (1976Obs....96..153G).
HD 200905 No sign of the secondary in the near-UV. Spectral type of A1.5 from 
HD 200905  Parsons & Ake (1998, Cat. <J/ApJS/119/83>). Our photometric model 
HD 200905  shows {Delta}Mv=5.6, which is the same as Parsons & Ake give.
HD 202447 Am (A4, A5, F0).
HD 205114 Supergiant G primary: see Sect. 5. Secondary type B7/B8.
HD 207218 The UV spectrum is almost purely that of the secondary 
HD 207218  (see Sect. 4.3.2).
HD 208816 VV Cep. No appropriate standard for subtraction.
HD 213310 Poor subtraction; B7/8 is uncertain. If earlier than B7, it could be a
HD 213310  shell star. Parsons & Ake (1998, Cat. <J/ApJS/119/83>) give B5+p.
HD 213503 The mass function, f(m)=1.75 (Griffin, 1990JApA...11..491G), implies 
HD 213503  a double secondary.
HD 214558 Probably Am (A5.5:, A8.5:, F0).
HD 215242 Hipparcos parallax very uncertain. Primary has deep lines in the IR, 
HD 215242  suggesting that the luminosity may be higher than III.
HD 215318 Low rotation; appears to be Am.
HD 218257 Closely resembles the MK standard HD 11636: see HD 11154. Possibly Am.
HD 218640 Could be a marginal Am.
HD 220636 Very high rotation; K line wide, plus a possible IS feature. 
HD 220636  Balmer lines indicate A1/2.
HD 223047 Supergiant G primary: see  Sect. 5. Secondary B9 to A0 (poor 
HD 223047  subtraction). Parsons & Ake (1998, Cat. <J/ApJS/119/83>) give B9p.
HD 223932 Poor-quality subtraction, so result doubtful; HD type is G5A3, and 
HD 223932  Houck & Smith-Moore (1988, Cat. <III/133>) give K0 III+A5/A7 V. 
HD 223932  High rotation, similar to HD 17878.
HD 224646 Classification difficult; K line is near A1 but the Balmer lines 
HD 224646  indicate B9. If B9, the K line must contain a remnant of the primary.
HD 224646  Its profile is unusual, and includes a small line that may be IS 
HD 224646  (see HD 13474).
HD 234138 No sign in the near-UV of a hot secondary, though Hynek 
HD 234138  (1938CoPer...1...10H) suspected it as composite.