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Query : 2015A&A...575A..50A |
2015A&A...575A..50A - Astronomy and Astrophysics, volume 575A, 50-50 (2015/3-1)
What causes the large extensions of red supergiant atmospheres? Comparisons of interferometric observations with 1D hydrostatic, 3D convection, and 1D pulsating model atmospheres.
ARROYO-TORRES B., WITTKOWSKI M., CHIAVASSA A., SCHOLZ M., FREYTAG B., MARCAIDE J.M., HAUSCHILDT P.H., WOOD P.R. and ABELLAN F.J.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: fundamental parameters - stars: individual: V602 Car - stars: individual: HD 95687 - stars: atmospheres - individual: HD 183589 - stars: supergiants
Simbad objects: 30
Number of rows : 30 |
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 | * omi Cet | Mi* | 02 19 20.79210 | -02 58 39.4956 | 7.63 | 6.53 | 5.03 | M5-9IIIe+DA | 1525 | 0 | ||
2 | * alf Tau | LP? | 04 35 55.23907 | +16 30 33.4885 | 4.32 | 2.40 | 0.86 | -0.37 | -1.31 | K5+III | 1255 | 2 |
3 | * alf Ori | s*r | 05 55 10.30536 | +07 24 25.4304 | 4.38 | 2.27 | 0.42 | -1.17 | -2.45 | M1-M2Ia-Iab | 1665 | 0 |
4 | V* VY CMa | s*r | 07 22 58.3261352189 | -25 46 03.194390594 | 12.01 | 10.068 | 8.691 | 7.938 | M5Iae | 1101 | 0 | |
5 | V* RW Vel | Mi* | 09 20 19.4216289288 | -49 31 30.538637292 | 10.92 | 8.90 | M7e | 35 | 0 | |||
6 | V* X Hya | Mi* | 09 35 30.2667472344 | -14 41 28.610073456 | 10.02 | 7.20 | 9.24 | M7-8+e | 151 | 0 | ||
7 | V* Z Car | Mi* | 10 13 54.5780798664 | -58 51 08.603411328 | 13.50 | M8 | 25 | 0 | ||||
8 | V* W Vel | Mi* | 10 15 14.8298044200 | -54 28 41.989481076 | 12.23 | 8.30 | M9 | 75 | 0 | |||
9 | * t01 Car | PM* | 10 36 20.5194125328 | -59 33 51.817814604 | 6.249 | 5.088 | K1III | 29 | 0 | |||
10 | HD 95687 | s*r | 11 01 35.7593300304 | -61 02 55.820385276 | 9.130 | 7.90 | M2Iab | 40 | 0 | |||
11 | HD 95686 | * | 11 01 44.8906220352 | -57 34 25.642242084 | 11.18 | 10.09 | K2 | 5 | 0 | |||
12 | Ass Car OB 2 | As* | 11 08 | -60.2 | ~ | 82 | 0 | |||||
13 | V* V602 Car | s*r | 11 13 29.9741868816 | -60 05 28.849300980 | 10.68 | 8.815 | M3Ia-Iab | 51 | 0 | |||
14 | * e Leo | * | 11 30 18.8933524920 | -03 00 12.598924644 | 8.14 | 6.31 | 4.77 | K3+IIIFe-0.5 | 142 | 0 | ||
15 | V* BK Vir | AB* | 12 30 21.0136448232 | +04 24 59.142255840 | 9.60 | 8.82 | 7.28 | M7-III: | 147 | 0 | ||
16 | * gam Hya | SB* | 13 18 55.2976891983 | -23 10 17.450424894 | 4.58 | 3.92 | 3.00 | 2.40 | 1.93 | G8IIIa | 178 | 0 |
17 | * alf Sco | s*r | 16 29 24.45970 | -26 25 55.2094 | 4.08 | 2.75 | 0.91 | -0.64 | -1.87 | M1.5Iab+B2Vn | 745 | 0 |
18 | V* AH Sco | s*r | 17 11 17.0194487616 | -32 19 30.714035556 | 10.03 | 8.10 | M5Ia-Iab | 136 | 0 | |||
19 | V* KW Sgr | s*r | 17 52 00.7269495408 | -28 01 20.555654448 | 11.45 | 11.00 | M3Ia | 89 | 0 | |||
20 | V* VX Sgr | s*r | 18 08 04.0442790744 | -22 13 26.600899044 | 11.72 | 9.41 | 6.52 | 3.90 | 2.11 | M8.5Ia | 594 | 0 |
21 | V* UY Sct | s*r | 18 27 36.5281722864 | -12 27 58.898573712 | 14.20 | 11.20 | 9.51 | 6.93 | M4Iae | 61 | 0 | |
22 | HD 183387 | * | 19 29 18.0225976176 | +00 14 45.867845796 | 7.541 | 6.245 | K2III | 19 | 0 | |||
23 | HD 183589 | * | 19 30 10.5351087360 | +02 54 14.663673360 | 7.839 | 6.042 | K5III | 30 | 0 | |||
24 | NGC 6803 | PN | 19 31 16.4826019750 | +10 03 21.620200381 | 13.034 | 11.616 | 13.242 | ~ | 248 | 0 | ||
25 | * mu. Aql | PM* | 19 34 05.3529921054 | +07 22 44.184329526 | 6.87 | 5.63 | 4.45 | 3.55 | 2.94 | K3-IIIbFe0.5 | 263 | 1 |
26 | V* NU Pav | LP* | 20 01 44.7454026 | -59 22 33.217740 | 7.97 | 6.66 | 5.13 | M6III | 67 | 0 | ||
27 | V* RS Cap | AB* | 21 07 15.4311630672 | -16 25 21.462156804 | 9.56 | 8.36 | M6/7III | 70 | 0 | |||
28 | * eps Oct | LP* | 22 20 01.6806230015 | -80 26 23.089683198 | 6.433 | 5.177 | M5III | 61 | 0 | |||
29 | * bet Peg | LP* | 23 03 46.45746 | +28 04 58.0336 | 6.05 | 4.09 | 2.42 | 0.92 | -0.40 | M2.5II-III | 593 | 1 |
30 | * psi Peg | ** | 23 57 45.5268071 | +25 08 29.047968 | 7.91 | 6.25 | 4.66 | 3.20 | 1.86 | M3III | 125 | 0 |
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