1997AJ....113.1666B

Query : 1997AJ....113.1666B

1997AJ....113.1666B - Astron. J., 113, 1666-1677 (1997)

The stellar populations of spiral disks. I. A new observational approach: description of the technique and spectral gradients for the inter-arm regions of NGC 4321 (M100).

BEAUCHAMP D. and HARDY E.

Journal keyword(s):

Simbad objects: 36

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Number of rows : 36
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 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
3 * gam Tau ** 04 19 47.6039239005 +15 37 39.511385129 5.46 4.64 3.65 4.83   G9.5IIIabCN0.5 569 0
4 * del Tau SB* 04 22 56.0951595936 +17 32 33.049802364 5.56 4.74 3.76 5.56   G9.5IIICN0.5 542 0
5 * 30 Gem PM* 06 43 59.2871476656 +13 13 40.799645724 6.82 5.65 4.49 3.63 3.03 K0+IIICa1 156 0
6 * 62 Aur PM* 06 59 02.8473250152 +38 03 08.346327696   7.245 6.021     K2III 90 0
7 * tau Gem PM* 07 11 08.3703137689 +30 14 42.589571474 7.08 5.68 4.42 3.45 2.82 K2III 175 1
8 * iot Gem ** 07 25 43.5956409143 +27 47 53.086950407 5.67 4.83 3.79 3.02 2.52 G9IIIb 222 0
9 * gam CMi SB* 07 28 09.7942869528 +08 55 31.888128216 7.26 5.73 4.30 3.19 2.40 K3-IIIFe-0.5 112 0
10 * del Cnc ** 08 44 41.0991810454 +18 09 15.509048595 6.01 5.02 3.94 3.16 2.62 K0+IIIb 212 0
11 * mu. Leo PM* 09 52 45.8170136628 +26 00 25.024269924 6.50 5.10 3.88 2.97 2.39 K2IIIbCN1Ca1 479 0
12 * n Leo SB* 11 15 51.8801100552 +13 18 27.234958860 7.61 6.52 5.32     K2III 167 0
13 HD 102328 * 11 46 55.6222860288 +55 37 41.480416020   6.528 5.254     K2.5IIIbCN1 169 0
14 M 100 AGN 12 22 54.9299993592 +15 49 20.296257960 10.04 10.05 9.35     ~ 1963 2
15 * 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
16 HD 122563 Pe* 14 02 31.8455084952 +09 41 09.944391876 7.47 7.10 6.19 5.37 4.79 G8:III:Fe-5 920 0
17 * 20 Boo PM* 14 19 45.2351074992 +16 18 25.010494488       4.1   K3III 163 0
18 * 31 Boo V* 14 41 38.7511938264 +08 09 42.352458552   5.866 4.862     G7IIIa 165 0
19 * del Boo PM* 15 15 30.1628200572 +33 18 53.392471806 5.12 4.44 3.49 2.76 2.25 G8IIIFe-1 388 0
20 * tet UMi V* 15 31 24.9136103328 +77 20 57.695859924   6.535 4.982     K5-IIICN0.5 126 0
21 * alf Ser PM* 15 44 16.0741095811 +06 25 32.268792881 5.080 3.800 2.630 1.82 1.25 K2IIIbCN1 533 0
22 * ome Ser PM* 15 50 17.5468226304 +02 11 47.432004216   6.236 5.217     K0IV 146 1
23 * kap CrB PM* 15 51 13.9312943632 +35 39 26.573691158 6.69 5.82 4.82 4.06 3.57 K1IVa 290 1
24 * phi Ser PM* 15 57 14.5708375584 +14 24 52.132920192   6.677 5.530     K2III+ 120 0
25 * eps CrB PM* 15 57 35.2514020181 +26 52 40.366652765 6.650 5.360 4.130 3.27 2.64 K2IIIab 280 1
26 * tau CrB PM* 16 08 58.3089242491 +36 29 27.134047440 6.64 5.75 4.73 4.01 3.47 K1-III-IV 195 0
27 HD 145148 PM* 16 09 11.2150771435 +06 22 43.289900623   6.97   5.3   K1.5IV 187 0
28 * sig CrB B PM* 16 14 40.3874065885 +33 51 27.096186894   7.04 6.42     G1V 146 0
29 * ksi CrB ** 16 22 05.8238662920 +30 53 31.185448080   5.833 4.849     G9IIIFe-0.5 136 0
30 * h Her PM* 16 32 36.2919789280 +11 29 16.948144457 8.16 6.34 4.85 3.65 2.79 K4.5III 164 0
31 * kap Oph LP? 16 57 40.0975028128 +09 22 30.104472450 5.52 4.36 3.20 2.36 1.82 K2III 314 0
32 * 71 Oph * 18 07 18.3593981592 +08 44 01.922061912   5.592 4.640     G8III 182 0
33 HD 167042 PM* 18 10 31.6398993768 +54 17 11.592196980   6.89   5.4   K1III 174 1
34 * kap Lyr V* 18 19 51.7091048595 +36 03 52.370938421 6.70 5.51 4.34 3.48 2.93 K2-IIIabCN0.5 150 0
35 HD 175743 PM* 18 56 06.1210399992 +18 06 19.475094852       5.0   K1III 78 0
36 * pi. Aql ** 19 48 42.0576531 +11 48 57.217672 6.520 6.230 5.740 6.58   G8III+A3V 71 0

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