Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.astro.spbu.ru/DOP/8-GLIB/uv/
Дата изменения: Fri Nov 19 12:10:04 2010
Дата индексирования: Mon Oct 1 22:39:16 2012
Кодировка:

Поисковые слова: п п п п п п п п п
Database of interstellar extinction and polarization curves

DATABASE OF INTERSTELLAR EXTINCTION AND POLARIZATION CURVES

This database contains information about the interstellar extinction and polarization curves observed in a wide spectral range from ultraviolet to infrared for stars located in different regions of the Galaxy and Magellanic Clouds.
The list of objects is naturally limitted by those stars for which the ultraviolet spectropolarimetric observations were performed.

ULTRAVIOLET SPECTROPOLARIMETRIC OBJECTS

(1)
UV/Vis
(2)
NAME
(3)
Name
(4)
l
(5)
b
(6)
CLASS
(7)
V
(8)
(B-V)
(9)
d(pc)
(10)
E(B-V)
(11)
PA
(12)
λmax
(13)
Pmax
(14)
P(6)
(15)
WLR(6)
(16)
ext
(17)
pol
(18)
depl
Wb/P HD2905 κ Cas 120.8 0.13 B1 Iae 4.16 0.14 880 0.33 83 0.50 1.51 0.696±0.017 0.57 dir dir dir
H/P BD+64 106 123.6 1.99 B1 V 10.34 0.69 96 0.60 5.52 3.60 1.11 dir dir dir
H/P HD7252 125.7 -1.86 B1 V 7.12 0.09 840 0.35 96 0.50 3.74 1.62 1.41 dir dir dir
W2/P HD24263 31 Tau 182.1 -34.87 B5 V 5.66 0.06 180 0.20 150 0.55 1.01 0.434±0.056 0.38 dir dir dir
W2/P HD24992 143.0 7.34 B3 III 8.03 0.05 137 0.48 5.68 2.620±0.185 2.38 dir dir dir
W2/P HD25090 143.2 7.34 B0.5 III 7.32 0.31 0.61 135 0.49 5.70 2.736±0.183 2.26 dir dir dir
W1/P HD25443 143.7 7.35 B0.5 III 6.74 0.34 810 0.61 135 0.50 5.17 3.359±0.115 1.94 dir dir dir
W2/P HD25638 HR1260 143.7 7.65 B0 II-III 6.93 0.46 0.61 141 0.45 6.31 3.833±0.185 3.08 dir dir dir
W2/P HD25940 48 Per 153.6 3.04 B3Ve 4.04 -0.03 106 0.16 173 0.57 0.97 0.252±0.021 0.24 dir dir dir
Wb/P HD30614 α Cam 144.1 14.04 O9.5Iae 4.29 0.03 138 0.47 1.58 0.895±0.022 0.70 dir dir dir
W2/P HD34078 AE Aur 172.1 -2.25 O9.5 V 5.96 0.22 610 0.52 161 0.56 1.83 0.555±0.087 0.48 dir dir dir
W1/P HD37903 206.9 -16.53 B1.5V 7.51 0.29 880 0.35 120 0.68 1.97 0.177±0.067 0.22 dir dir dir
Wb/A HD62542 255.9 -9.23 B3 V 8.04 0.17 400 0.33 26 0.59 1.43 0.647±0.195 0.31 dir dir dir
W2/W HD73882 260.2 0.64 O9 III 7.24 0.40 1100 0.71 165 0.65 1.86 0.248±0.152 0.26 dir dir dir
W2/W HD77581 Vela X1 263.1 3.92 B0.5 Ibe 6.89 0.47 1200 0.69 84 0.55 3.99 2.094±0.134 1.12 dir dir dir
W2/M HD94963 289.8 -1.81 O6.5 III(f) 7.15 -0.10 2190 0.24 108 0.55 0.47 0.307± dir dir dir
H/- HD98695 295.9 -10.37 B4 V 6.41 0.05 250 0.23 115 0.60 2.20 0.40 0.44 dir dir dir
W1/A HD99264 296.3 -10.51 B2 IV-V 5.59 0.06 390 0.30 120 0.55 2.65 0.619±0.050 0.74 dir dir dir
W1/A HD113904 θ Mus 304.7 -2.49 B0Ia+WC5 5.50 -0.09 1800 0.20 79 0.55 1.54 0.416±0.054 0.43 dir dir dir
W2/P HD147084 σ Sco 352.3 18.05 A4 II-III 4.55 0.83 30 0.70 4.48 0.72±0.40 0.43 dir dir dir
W2/P HD147888 ρ Oph D 353.6 17.7 B5 V 6.74 0.31 54 0.68 3.51 0.454±0.074 0.39 dir dir dir
W2/P HD147933 ρ Oph AB 353.7 17.68 B2 IV-V 4.59 0.22 190 0.48 49 0.69 2.71 0.279±0.017 0.28 dir dir dir
G/P HD149757 ζ Oph 6.3 23.58 O9.7 2.56 0.02 0.59 1.43 dir dir dir
W2/P HD161056 18.7 11.58 B1.5 V 6.30 0.37 290 0.63 67 0.59 4.01 0.834±0.111 0.87 dir dir dir
W2/P HD161961 23.6 12.9 B0 III 7.81 0.22 1500 0.51 78 0.53 2.66 0.568±0.119 0.84 dir dir dir
W2/P HD188220 25.3 -20.99 A0 V 7.90 0.10 220 0.38 171 0.61 2.34 dir dir dir
W2/P HD189957 77.4 6.17 O9.5 III 7.81 0.01 2190 0.31 146 0.20 dir dir dir
Wb/P HD193237 P Cyg 75.8 1.31 B1 Iape 4.82 0.42 40 0.41 1.69 0.418±0.051 0.99 dir dir dir
W2/P HD193682 75.9 0.82 O5e 8.41 0.51 1800 0.83 67 0.32 0.78 0.530±0.301 0.63 dir dir dir
Wb/P HD197770 93.9 9 B2 III 6.32 0.33 420 0.57 131 0.49 3.88 1.464±0.056 1.54 dir dir dir
H/P HD204827 99.2 5.55 B0 V 7.95 0.80 610 1.10 58 0.43 5.62 3.84 3.01 dir dir dir
W2/P HD207198 103.1 6.99 O9 IIe 5.95 0.31 1000 0.62 27 0.41 0.98 0.822±0.066 0.57 dir dir dir
W2/P HD216658 109.6 2.35 B0 V 9.29 0.72 105 0.55 5.66 1.64±0.37 1.58 dir dir dir
W2/P HD216898 109.9 2.39 O8 8.02 0.53 1000 0.85 85 0.53 4.18 1.04±0.201 1.32 dir dir dir
W2/P HD217490 109.3 -0.26 B0.5 Ia 8.73 0.80 2400 1.02 52 0.44 3.88 1.63 dir dir dir

The work was supported by the RFBR grant 07-02-00831.