1996A&AS..116..239D


Query : 1996A&AS..116..239D

1996A&AS..116..239D - Astron. Astrophys., Suppl. Ser., 116, 239-248 (1996/April-2)

A library of H band stellar spectra for stellar population analysis purposes.

DALLIER R., BOISSON C. and JOLY M.

Abstract (from CDS):

A sample of 37 stars of luminosity classes I, III, V, including few SMR stars observed in the H band with a medium resolution (R=1500-2000) is presented. This sample of flux calibrated spectra is intended to widen existing stellar libraries. A new IR spectrograph, ISIS/IR, foreseen for CFHT has been used. Its main characteristics are briefly described. Stellar spectra obtained with this new spectrograph are compared to similar data obtained with the ESO NTT IRSPEC spectrograph. The behaviour of some prominent features is described and it is shown that the COλ1.60/SiIλ1.60 line ratio is a good luminosity indicator for stellar types later than K0.

Abstract Copyright: ∼

Journal keyword(s): line: identification - stars: fundamental parameters: classification - stars: late type - Infrared: stars - atlases

VizieR on-line data: <Available at CDS (J/A+AS/116/239): tables 1,2,3 and FITS files>

Simbad objects: 39

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Number of rows : 39
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 * 12 Per SB* 02 42 14.9145674304 +40 11 38.221732500 5.65 5.51 4.92 4.42 4.12 F9V 193 0
2 * o Per * 03 42 22.6459308614 +33 57 54.093701142 4.13 4.912 4.972     B0.5V 315 0
3 HD 22764 * 03 42 42.7369929720 +59 58 09.802899408 9.32 7.54 5.78 4.46 3.44 K3.5IIIb+G 62 0
4 * gam Ori V* 05 25 07.86325 +06 20 58.9318 0.54 1.42 1.64 1.73 1.95 B2III 542 1
5 * lam Ori A Em* 05 35 08.2760807112 +09 56 02.991326316 2.17 3.48 3.47     O8III((f)) 527 0
6 * 15 Mon Be* 06 40 58.65963 +09 53 44.7229 3.360 4.45 4.68   4.88 O7V+B1.5/2V 823 0
7 HD 55775 * 07 14 10.8500851992 -03 54 06.401226168   7.55 5.94     K5III 28 0
8 * 145 CMa s*r 07 16 36.8345570496 -23 18 56.138269860 8.37 6.50 4.79 3.47 2.51 K3Ib- 100 0
9 V* MZ Pup s*r 08 04 16.1895113976 -32 40 29.389546632 9.00 7.06 5.12     M1Iab-Ib 44 0
10 V* AB Pyx s*r 08 30 29.7960828288 -36 43 16.789857024   8.665 6.783     M3-Iab-Ib 37 0
11 * F Hya * 08 43 40.3744846779 -07 14 01.422508229   5.441 4.625     G1Ib 172 0
12 * ups01 Hya * 09 51 28.6749789221 -14 50 47.863368049 5.68 5.03 4.11 3.42 2.95 G7III 166 0
13 BD-03 2870 PM* 10 12 17.6682499584 -03 44 44.392042932 11.941 10.757 9.264 8.258 7.066 M2V 283 1
14 * 46 Leo LP* 10 32 11.7734449491 +14 08 14.170878403 9.18 7.14 5.46     M1III 103 0
15 * rho Leo s*b 10 32 48.6703908997 +09 18 23.705339948 2.780 3.720 3.870 3.90 4.06 B1Iab 550 0
16 * gam Cha V* 10 35 28.1055499388 -78 36 28.038741243 7.65 5.70 4.12 2.86 1.88 K4III 85 0
17 HD 93800 PM* 10 49 31.6945155936 -06 46 10.495954272   10.00 9.10     K1III 34 0
18 * 90 Leo ** 11 34 42.49024 +16 47 48.8956 5.150 5.780 5.940     B6.6(IV)+B3.7(V) 152 0
19 HD 103095 Pe* 11 52 58.7673387755 +37 43 07.254113125 7.38 7.20 6.45 5.80 5.35 K1V_Fe-1.5 842 1
20 * 31 Crt SB* 12 00 51.1591616208 -19 39 32.332235148   5.080 5.264     B2IV 125 0
21 * rho Cen Pu* 12 11 39.1197479712 -52 22 06.384420264 3.20 3.81 3.96 4.05 4.21 B3V 136 0
22 * c Vir RG* 12 20 20.9813922197 +03 18 45.255217001 7.27 6.12 4.96 4.07 3.46 K0.5IIIbFe-0.5 380 0
23 HD 109655 * 12 35 53.0952076080 +45 46 51.499913448   8.92 7.3     K5III 31 0
24 HD 111180 * 12 47 07.7356927080 +32 34 03.802751436   9.24 7.73     K5III-IV 22 0
25 * 31 Com Ro* 12 51 41.9201696640 +27 32 26.565016812 5.81 5.61 4.94 4.39 4.04 G0IIIp 443 1
26 * psi Vir LP* 12 54 21.1630369857 -09 32 20.360128902 7.94 6.39 4.80 3.23 1.95 M3-III 173 0
27 HD 112758 ** 12 59 01.5612841731 -09 50 02.679322421 8.737 8.384 7.588 7.163 6.729 G9V 196 1
28 * bet Com PM* 13 11 52.3938268062 +27 52 41.462309460 4.92 4.84 4.25 3.77 3.47 F9.5V 946 0
29 HD 115404 PM* 13 16 51.0514297623 +17 01 01.840901307   7.69 6.66     K2V 316 0
30 * gam Hya SB* 13 18 55.2976891983 -23 10 17.450424894 4.58 3.92 3.00 2.40 1.93 G8IIIa 192 0
31 * alf Vir bC* 13 25 11.57937 -11 09 40.7501 -0.20 0.74 0.97 1.06 1.30 B1V 877 1
32 * kap Vir PM* 14 12 53.7448526298 -10 16 25.332461336 7.00 5.53 4.21 3.14 2.39 K2.5IIIFe-0.5 149 0
33 HD 130871 PM* 14 50 20.9570288027 +06 48 53.748865230   10.06   8.5   K3 98 0
34 HD 134468 s*r 15 13 01.0209623064 -61 44 37.596772464   8.126 6.269     K4Ib 28 0
35 * 42 Lib * 15 40 16.8973226160 -23 49 05.101136148 7.80 6.29 4.96 4.00 3.32 K3-IIICN2 121 0
36 HD 157881 PM* 17 25 45.2324302566 +02 06 41.123732402 10.126 8.865 7.56 6.649 5.89 K7V 361 0
37 * mu. Ara PM* 17 44 08.7031414872 -51 50 02.591603160   5.85 5.15     G3IV-V 578 2
38 * alf Sct PM* 18 35 12.4271571798 -08 14 38.653839451 6.70 5.17 3.83 2.86 2.18 K3III 189 0
39 HD 175674 Pe* 18 58 52.9931784000 -48 30 21.255716988   8.52 7.84     K3III_Ba 54 0

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