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Query : 2007ApJ...671.2017R |
2007ApJ...671.2017R - Astrophys. J., 671, 2017-2027 (2007/December-3)
Mid-infrared interferometry of dust around massive evolved stars.
RAJAGOPAL J., MENUT J.-L., WALLACE D., DANCHI W.C., CHESNEAU O., LOPEZ B., MONNIER J.D., IRELAND M. and TUTHILL P.G.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: individual (AG Car) - stars: individual (NaSt 1) - stars: individual (WR 95) - stars: individual (WR 106) - Techniques: Interferometric
Simbad objects: 21
Number of rows : 21 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | * alf Hya | * | 09 27 35.24270 | -08 39 30.9583 | 5.14 | 3.42 | 1.97 | 0.93 | 0.16 | K3IIIa | 434 | 1 |
2 | * eta Car | Em* | 10 45 03.545808 | -59 41 03.95124 | 6.37 | 7.03 | 6.48 | 6.123 | 4.41 | LBV | 2440 | 0 |
3 | V* AG Car | WR* | 10 56 11.5781414448 | -60 27 12.810673260 | 7.00 | 7.57 | 6.96 | 7.73 | WN11h | 631 | 0 | |
4 | * eps Cru | PM* | 12 21 21.6081337639 | -60 24 04.133270061 | 4.98 | 3.57 | K3III | 90 | 0 | |||
5 | * c01 Cen | PM* | 14 43 39.4375747161 | -35 10 25.206876063 | 5.41 | 4.04 | K3IIIb | 70 | 0 | |||
6 | * kap Lib | PM* | 15 41 56.7924203448 | -19 40 43.654786104 | 8.24 | 6.30 | 4.72 | 3.44 | 2.50 | M0-IIIb | 79 | 0 |
7 | MR 74 | WR* | 17 36 19.8953017656 | -33 26 12.271864344 | 16.01 | 14.87 | 13.18 | 12.99 | WC9 | 90 | 1 | |
8 | WR 98a | WR* | 17 41 13.0411858104 | -30 32 30.409373688 | 18.40 | 15.20 | 13.82 | WC8/9 | 106 | 1 | ||
9 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 14415 | 0 | |||||
10 | NAME Quintuplet Cluster | OpC | 17 46 13.9 | -28 49 48 | ~ | 526 | 0 | |||||
11 | MR 80 | WR* | 18 02 04.1244400656 | -23 37 42.168277056 | 15.002 | 13.155 | 12.056 | WC9 | 229 | 1 | ||
12 | HD 313643 | WR* | 18 04 43.6647313968 | -21 09 30.555411624 | 13.58 | 13.27 | 12.02 | 11.67 | WC9d | 93 | 0 | |
13 | * gam02 Sgr | PM* | 18 05 48.4880988 | -30 25 26.723458 | 4.77 | 4.00 | 2.99 | 2.26 | 1.75 | K0+III | 148 | 0 |
14 | WR 112 | WR* | 18 16 33.4909366272 | -18 58 42.341845368 | 20.7 | 17.7 | WC8+O6/7III/V | 135 | 0 | |||
15 | * eta Ser | PM* | 18 21 18.6004923875 | -02 53 55.780691633 | 4.84 | 4.19 | 3.25 | 2.55 | 2.05 | K0III-IV | 377 | 0 |
16 | * lam Sgr | PM* | 18 27 58.2407185 | -25 25 18.114589 | 4.75 | 3.85 | 2.81 | 2.06 | 1.50 | K1IIIb | 277 | 0 |
17 | LS IV +00 5 | WR* | 18 52 17.5478270448 | +00 59 44.304835128 | 13.77 | 12.25 | WN10 | 45 | 0 | |||
18 | * tau Sgr | PM* | 19 06 56.4031131168 | -27 40 13.496293992 | 5.65 | 4.51 | 3.31 | 2.44 | 1.85 | K1.5IIIb | 157 | 0 |
19 | HD 192641 | WR* | 20 14 31.7666855880 | +36 39 39.598210224 | 7.80 | 8.20 | 7.91 | WC7pd+O9V | 330 | 0 | ||
20 | * alf02 Cap | PM* | 20 18 03.2555957142 | -12 32 41.467632703 | 5.20 | 4.51 | 3.58 | 2.91 | 2.42 | G9III | 170 | 0 |
21 | HD 193793 | WR* | 20 20 27.9757908696 | +43 51 16.286840244 | 6.90 | 7.25 | 6.85 | 4.58 | WC7pd+O5.5fc | 710 | 0 |
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