1993ApJ...414..740D

Query : 1993ApJ...414..740D

1993ApJ...414..740D - Astrophys. J., 414, 740-758 (1993/September-1)

Evidence for a dispersion in the lithium abundances of extreme halo stars.

DELIYANNIS C.P., PINSONNEAULT M.H. and DUNCAN D.K.

Abstract (from CDS):


Abstract Copyright: ∼

Journal keyword(s): Nuclear Reactions, Nucleosynthesis, Abundances - Stars: Abundances - Stars: Population II

Simbad objects: 32

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Number of rows : 32
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 BD-10 388 Pe* 01 50 32.6462570064 -09 21 02.840259744   10.78 10.4     F3 102 0
2 BD+09 352 ** 02 41 13.6396003457 +09 46 12.100750635 10.37 10.62 10.1 10.0   kA7.5hF8 109 0
3 G 4-37 Pe* 02 44 35.0876406984 +08 28 50.094009408   11.90 11.4 11.0   F7 96 0
4 HD 19445 Pe* 03 08 25.5883873084 +26 19 51.400965175 8.29 8.52 8.06 7.60 7.27 G2VFe-3 801 0
5 HD 284248 Pe* 04 14 35.5161858536 +22 21 04.252516252 9.49 9.68 9.23 8.77 8.43 sdG0 200 0
6 BD+03 740 HB* 05 01 16.6226363256 +04 06 37.021736844 9.97 10.17 9.7 9.6   sdF0 182 0
7 BD+24 1676 Pe* 07 30 41.2662525096 +24 05 10.248524088   11.15 10.7 10.4   F 139 0
8 HD 74000 Pe* 08 40 50.8036114756 -16 20 42.516208237 9.84 10.09 9.66     F2 279 0
9 HD 76932 PM* 08 58 43.9327642391 -16 07 57.817644364 6.47 6.39 5.86     G2VFe-1.8CH-1 426 0
10 Ross 889 Pe* 09 40 43.2053340378 +01 00 29.511836741       10.39   sdA4 166 0
11 HD 84937 Pe* 09 48 56.0992891997 +13 44 39.326709913 8.49 8.68 8.32 7.97 7.70 F8Vm-5 831 0
12 BD+29 2091 PM* 10 47 23.1623890044 +28 23 55.925628075   10.72   10.1   F5 151 0
13 HD 108177 PM* 12 25 34.9568267745 +01 17 02.259553591 9.87 10.09 9.66 9.21 8.89 F0V 266 0
14 Wolf 1447 Pe* 12 34 25.1299405728 +15 16 48.959531004   12.385 11.976 11.676 11.378 A6 73 0
15 G 238-30 Pe* 13 17 40.1964559089 +64 15 12.170254208   13.91 12.9 12.4   sdA8 53 1
16 Wolf 1492 Pe* 13 40 02.4921849768 -00 02 18.750053436 11.601 11.832 11.451 11.184 10.892 sdF0: 299 0
17 BD+34 2476 PM* 13 59 09.4837849799 +33 51 39.379962282 10.25 10.44   9.7   sdF5 167 0
18 G 201-5 PM* 14 36 08.3666970497 +55 33 04.605415573   11.93   11.1   sdF6 45 0
19 BD+26 2606 SB* 14 49 02.3593347728 +25 42 09.192358874 9.92 10.16 9.73 9.27 8.95 A5 383 0
20 HD 132475 PM* 14 59 49.7651173448 -22 00 45.815162806 8.98 9.11 8.55     F5/6V 256 1
21 HD 134169 SB* 15 08 18.0570477216 +03 55 50.144061360 8.14 8.22 7.70     F7V 220 0
22 HD 140283 Pe* 15 43 03.0971190219 -10 56 00.595693188 7.508 7.711 7.212 6.63 8.21 F9VkA5mA1 985 0
23 BD+42 2667 Pe* 16 03 13.2988107325 +42 14 46.651500150   10.33   9.6   F5 159 0
24 BD+02 3375 Pe* 17 39 45.5948675731 +02 24 59.606824535 10.18 10.40 9.92 9.47 9.12 A5 205 0
25 HD 160617 Pe* 17 42 49.3234249010 -40 19 15.503834657   9.18 8.7 8.394 8.065 G0 220 0
26 BD+20 3603 Pe* 17 54 43.2306198848 +20 16 16.444611703   10.13 9.8 9.6   F0 169 0
27 HD 345957 PM* 20 10 48.1625876064 +23 57 54.510596568   9.36   8.6   G0V: 150 0
28 HD 194598 PM* 20 26 11.9183775668 +09 27 00.429558608 8.62 8.82 8.34 7.90 7.56 F8 315 0
29 BD+17 4708 SB* 22 11 31.3756832854 +18 05 34.177983548 9.73 9.91 9.46 9.03 8.70 sdF8 580 0
30 HD 219617 ** 23 17 05.04375 -13 51 03.5971 8.41 8.60 8.14 7.70 7.37 F8 317 0
31 BD+02 4651 PM* 23 19 40.4500387773 +03 22 16.694733495   10.67   9.9   sdF6 117 0
32 BD+59 2723 SB* 23 26 32.8574602006 +60 37 42.846968726 10.74 10.92   10.1   sdF8 111 0

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