1997A&A...325..693M

Query : 1997A&A...325..693M

1997A&A...325..693M - Astronomy and Astrophysics, volume 325693-699 (1997/9-2)

Quantitative spectral classification based on photoelectric spectrum scanner measurements of F-K stars.

MALYUTO V. and SCHMIDT-KALER T.

Abstract (from CDS):

New criteria of quantitative spectral classification have been introduced and the method of stepwise linear regression to these criteria for quantitative spectral classification of F-K stars has been applied to the Bochum photoelectric spectra.

Abstract Copyright: ∼

Journal keyword(s): stars: fundamental parameters, classification

VizieR on-line data: <Available at CDS (J/A+A/325/693): table4>

Simbad objects: 54

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Number of rows : 54
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * bet Hyi PM* 00 25 45.07036 -77 15 15.2860 3.52 3.41 2.79 2.28 1.94 G0V 631 0
2 * eta Psc ** 01 31 29.0081880156 +15 20 44.994632991 5.320 4.600 3.620 2.90 2.40 G7IIIa 255 0
3 * tau Cet PM* 01 44 04.0831371922 -15 56 14.927607677 4.43 4.22 3.50 2.88 2.41 G8V 1354 1
4 * alf Hyi PM* 01 58 46.1385834212 -61 34 11.359751511 3.33 3.13 2.84 2.55 2.39 F0IV 225 0
5 * sig Cet ** 02 32 05.1877984910 -15 14 41.653561505 5.19 5.20 4.75 4.34 4.07 F5V 217 0
6 * zet02 Ret ** 03 18 12.8188824117 -62 30 22.904711032   5.814 5.228     G1V 399 0
7 * kap01 Cet BY* 03 19 21.6964175772 +03 22 12.714979884 5.71 5.52 4.85 4.27 3.91 G5V 948 0
8 * e Eri PM* 03 19 55.6509122226 -43 04 11.215188426 5.20 4.98 4.27 3.65 3.25 G6V 501 1
9 * 10 Tau PM* 03 36 52.3837044168 +00 24 05.992097829 5.23 5.15 4.30 4.09 3.77 F9IV-V 595 0
10 * 46 Tau ** 04 13 33.0904461000 +07 42 58.017467664 5.65 5.65 5.29 4.94 4.75 F2V 172 0
11 * alf Ret PM* 04 14 25.4700044050 -62 28 25.692560378 4.90 4.27 3.36 2.71 2.27 G8IIIa: 129 0
12 * omi02 Eri PM* 04 15 16.3196189945 -07 39 10.330779018 5.69 5.25 4.43 3.74 3.29 K0V 879 0
13 * pi.03 Ori PM* 04 49 50.4112051485 +06 57 40.600622266 3.620 3.630 3.190 2.77 2.51 F6V 601 0
14 * eps Lep PM* 05 05 27.6644072506 -22 22 15.724153311 6.41 4.64 3.18 2.08 1.27 K4III 169 0
15 * bet Lep PM* 05 28 14.7228880318 -20 45 33.997988694 4.13 3.66 2.84 2.19 1.75 G5II-IIIa: 254 0
16 * alf Lep V* 05 32 43.8161188 -17 49 20.241380 3.02 2.77 2.57 2.35 2.14 F0Ib 289 0
17 * gam Lep PM* 05 44 27.7906169580 -22 26 54.187756254 4.08 4.07 3.60 3.15 2.89 F6V 459 0
18 * eta Lep PM* 05 56 24.2934904501 -14 10 03.718335613 4.05 4.05 3.72 3.39 3.23 F2V 352 0
19 * alf Car * 06 23 57.10988 -52 41 44.3810 -0.49 -0.59 -0.74 -0.96 -1.13 A9II 461 1
20 * omi01 CMa s*r 06 54 07.9522701192 -24 11 03.159501504 7.59 5.60 3.87 2.70 1.88 K2Iab 185 0
21 * del CMa s*y 07 08 23.4840514 -26 23 35.518484 3.06 2.52 1.84 1.33 1.00 F8Ia 348 0
22 * alf CMi SB* 07 39 18.11950 +05 13 29.9552 0.82 0.79 0.37 -0.05 -0.28 F5IV-V+DQZ 1925 0
23 * ksi Pup * 07 49 17.6535518440 -24 51 35.221966694 5.72 4.56 3.30 2.43 1.88 G6Ib 201 0
24 * zet Mon * 08 08 35.6480975954 -02 59 01.635577977 6.02 5.30 4.33 3.60 3.11 G2Ib 152 0
25 * bet Cnc PM* 08 16 30.9209888482 +09 11 07.958245527 6.750 5.000 3.520 2.42 1.62 K4IIIBa0.5: 383 0
26 * bet Pyx * 08 40 06.1432829632 -35 18 30.078413177   4.885 3.954     G5II/III 82 0
27 * gam Pyx PM* 08 50 31.9225999562 -27 42 35.429733075 6.67 5.27 4.01 3.06 2.39 K2.5III 122 0
28 * zet Hya PM* 08 55 23.6261974442 +05 56 44.034757439 4.92 4.10 3.10 2.39 1.90 G8.5III 254 0
29 * lam Vel s*r 09 07 59.75787 -43 25 57.3273 5.67 3.86 2.21 0.97 0.03 K4Ib 230 0
30 * k Vel * 09 15 45.0797665800 -37 24 47.317883724 5.17 5.07 4.62 4.24 3.96 F3/5V 83 0
31 * alf Hya * 09 27 35.24270 -08 39 30.9583 5.14 3.42 1.97 0.93 0.16 K3IIIa 455 1
32 * eps Leo V* 09 45 51.0736168507 +23 46 27.313597604 4.23 3.79 2.98 2.36 1.93 G1IIIa 354 0
33 * q Car LP* 10 17 04.9755364660 -61 19 56.296709026   4.899 3.350     K2.5II 147 0
34 V* V399 Car Ce* 10 27 24.4704883920 -57 38 19.698397044 5.29 5.18 4.70 4.10 3.62 A9/F0Ia/ab 143 0
35 * s Car V* 10 27 52.7297730743 -58 44 21.862230028   4.111 3.810     F2II 96 0
36 * r Car V* 10 35 35.2978599894 -57 33 27.480964912   6.043 4.430     K3II-IIb 39 0
37 * omi01 Cen LP* 11 31 46.0686288120 -59 26 31.418490516   6.134 5.097 4.31 3.64 G3_0-Ia 83 0
38 V* V810 Cen LP* 11 43 31.1923164072 -62 29 21.827165856 6.18 5.83 5.03 4.27 3.91 G0_0-IaFe1 158 0
39 HD 102365 PM* 11 46 31.0725331317 -40 30 01.285867174 5.65 5.55 4.88 4.35 3.97 G2V 378 1
40 * bet Vir PM* 11 50 41.7185158616 +01 45 53.001539131 4.26 4.15 3.60 3.13 2.85 F9V 973 0
41 * eps Crv PM* 12 10 07.4805825 -22 37 11.161983 5.79 4.32 2.98 2.05 1.41 K2+IIIa 158 0
42 * bet Crv PM* 12 34 23.2349224335 -23 23 48.336778328 4.17 3.52 2.64 2.03 1.59 G5IIBa0.3 272 0
43 * eps Vir PM* 13 02 10.5970152536 +10 57 32.935398266 4.45 3.71 2.79 2.16 1.71 G8III-IIIb 574 0
44 * 61 Vir PM* 13 18 24.3139864471 -18 18 40.297748582 5.710 5.440 4.740     G6.5V 742 1
45 * 70 Vir PM* 13 28 25.8085908881 +13 46 43.638308807 5.930 5.680 4.970 4.37 3.98 G4Va 754 1
46 * eta Boo SB* 13 54 41.07892 +18 23 51.7946 3.440 3.250 2.680 2.24 1.95 G0IV 733 0
47 * tet Cen PM* 14 06 40.94752 -36 22 11.8371 3.94 3.04 2.05 1.29 0.76 K0-IIIb 262 1
48 * alf Boo RG* 14 15 39.67207 +19 10 56.6730 2.46 1.18 -0.05 -1.03 -1.68 K1.5IIIFe-0.5 2417 1
49 * alf Cen A SB* 14 39 36.49400 -60 50 02.3737 0.96 0.72 0.01     G2V 1352 1
50 * lam Ser PM* 15 46 26.6142121632 +07 21 11.047378824 5.13 5.03 4.42 3.92 3.60 G0-V 618 0
51 * del TrA * 16 15 26.2707862589 -63 41 08.453417447   4.943 3.839     G2Ib-IIa 108 0
52 * gam Aps PM* 16 33 27.0825153352 -78 53 49.733407072   4.783 3.854     G8III 102 0
53 V* V2215 Oph RS* 17 16 13.3624141798 -26 32 46.136563394   7.50 6.34   4.8 K5V 334 0
54 * mu.01 Her ** 17 46 27.5472960785 +27 43 14.560978925 4.56 4.17 3.42 2.89 2.51 G5IV 719 0

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