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Home All issues Volume 508 / No 2 (December III 2009) A&A, 508 2 (2009) 909-922 Full HTML
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Table 1:

Log of the observations and spectral classification.

Name 		Var. Type Date Exp. Spectral Type
HIP BD HD GCVS   (*) (s)  
35 810 -03$^\circ$1873 57 884 V758 Mon Lb 1 3000 N (9), R8 (12)
36 623 +24$^\circ$1686 59 643 NQ Gem SR 1 3600 R9 (12), R6 (9), R8 (15)
39 118 - - - - 1 3600 R2 (15)
44 812 - 78 278 - - 1 3600 R6 (9), R5 (15)
53 832 +41$^\circ$2150 - - - 1 3600 R0 (15), CH-like (16), CH (2)
58 786 +71$^\circ$600 - - - 1 3600 R2 (15), CH-like (17), CH (2)
62 401 +04$^\circ$2651a 111 166 RU Vir Mira 1 3600 R3 (9), R3 (15)
62 944 - 112 127 - - 1 2400 K0 (13), K1 (14), K2 (11, 8, 10), K3 (7), R3 (1)
69 089 - 123 821 - - 1 3600 G9 (7), G8 (11), R2 (4), R2 (1)
74 826 +30$^\circ$2637 - - - 1 2700 R0 (12)
82 184 +23$^\circ$2998 - - - 3 3600 R0 (15), R2 (1)
84 266 +42$^\circ$2811 156 074 - - 2 2400 R0 (11, 17), R1 (5), R2 (1)
85 750 +02$^\circ$3336 - - - 3 3600 R2 (15), CH-like (17), N5 (4), N4 (1)
86 927 +17$^\circ$3325 - - - 2 3000 R0 (12)
87 603 - 163 838 -   3 5400 R3 (9), R5 (15)
88 887 +09$^\circ$3576 166 097 - - 2 3600 R4 (9), R5 (15)
91 929 -13$^\circ$5083 173 138 RV Sct Lb 3 3600 R3 (9), R3 (15), R4 (1)
94 049 -17$^\circ$5492 178 316 - - 3 5400 R4 (12), R2 (9)
95 422 - - - - 3 5400 R5 (15)
98 223 -00$^\circ$3883 188 934 - - 3 7200 R8 (12), R4 (9)
108 205 +49$^\circ$3673 208 512 LW Cyg Lb 3 4200 R3 (9), R2 (15), R8 (3)
109 158 - - CT Lac SRa 3 5400 R (6), N8 (3)
113 150 - 216 649 - - 3 3300 R3 (9), R5 (15)

* (1) 2003 March 12, 13; (2) 2003 August 9-10; (3) 2004 July 1-4.
References for the spectral types:
1: Barnbaum et al. (1996); 2: Bartkevicius (1996); 3: Eglitis et al. (2003); 4: Keenan (1993); 5: Keenan & Morgan (1941); 6: Lee & Bartlett (1944); 7: McClure (1970); 8: Morgan & Keenan (1973); 9: Sanford (1944); 10: Schild (1973); 11: Schmitt (1971); 12: Shane (1928); 13: Stock & Welhau (1956); 14: Upgren (1962); 15: Vandervort (1958); 16: Yamashita (1972); 17: Yamashita (1975).
The following stars show evidence of binarity:
HIP 36 623 (Carquillat & Prieur 2008), HIP 109 158 (Makarov & Kaplan 2005), HIP 53 832 (Platais et al. 2003) and HIP 85 750 (McClure 1997).

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