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Query : 2008MNRAS.390..377Z |
2008MNRAS.390..377Z - Mon. Not. R. Astron. Soc., 390, 377-382 (2008/October-2)
Rotational velocities of the giants in symbiotic stars - III. Evidence of fast rotation in S-type symbiotics.
ZAMANOV R.K., BODE M.F., MELO C.H.F., STATEVA I.K., BACHEV R., GOMBOC A., KONSTANTINOVA-ANTOVA R. and STOYANOV K.A.
Abstract (from CDS):
As a result of the rapid rotation, the cool giants in symbiotics should have 3-30 times larger mass-loss rates. Our results suggest also that bipolar ejections in symbiotics seem to happen in objects where the mass donors rotate faster than the orbital period.
All spectra used in our series of papers can be obtained upon request from the authors.
Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): binaries: symbiotic - stars: late-type - stars: rotation
Simbad objects: 43
Number of rows : 43 |
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 | * 30 Psc | LP? | 00 01 57.6194717328 | -06 00 50.654004048 | 7.88 | 6.04 | 4.41 | 2.85 | 1.44 | M3III | 140 | 0 |
2 | LIN 358 | Sy* | 00 59 12.2513835168 | -75 05 17.615251932 | 16.82 | 15.34 | 14.90 | 13.77 | K/Me | 47 | 0 | |
3 | * bet And | PM* | 01 09 43.92388 | +35 37 14.0075 | 5.58 | 3.62 | 2.05 | 0.81 | -0.19 | M0+IIIa | 555 | 1 |
4 | * psi Phe | LP* | 01 53 38.7393120868 | -46 18 09.609378142 | 7.71 | 6.00 | 4.41 | 2.68 | 1.17 | M4III | 108 | 0 |
5 | * rho02 Ari | LP* | 02 55 48.4979998 | +18 19 53.902936 | 8.56 | 7.44 | 5.93 | 3.51 | 1.34 | M6-III: | 224 | 0 |
6 | * alf Cet | LP? | 03 02 16.77307 | +04 05 23.0596 | 6.10 | 4.17 | 2.53 | 1.18 | 0.02 | M1.5IIIa | 461 | 1 |
7 | HD 42787 | LP* | 06 12 59.5727411832 | +06 00 58.528582956 | 8.063 | 6.459 | M2III | 25 | 0 | |||
8 | HD 46784 | * | 06 35 28.7901699624 | +05 30 45.267994728 | 9.74 | 8.01 | M1.5III | 30 | 0 | |||
9 | V* BX Mon | Sy* | 07 25 22.7621421120 | -03 35 50.644134204 | 12.27 | 11.24 | 10.92 | M5/6IIIe | 115 | 1 | ||
10 | EM* MWC 560 | Sy* | 07 25 51.2842107720 | -07 44 08.084175396 | 10.01 | 9.70 | 10.60 | M4ep+Beq | 208 | 0 | ||
11 | WRAY 15-157 | Sy* | 08 06 34.8733223088 | -28 32 01.223447100 | 10.0 | 7.4 | G5III | 24 | 0 | |||
12 | EM* AS 201 | PN | 08 31 42.8828281680 | -27 45 31.543524864 | 13 | 11.80 | F9III | 89 | 0 | |||
13 | * gam Cha | V* | 10 35 28.1055499388 | -78 36 28.038741243 | 7.65 | 5.70 | 4.12 | 2.86 | 1.88 | K4III | 79 | 0 |
14 | * 72 Leo | LP* | 11 15 12.2283936624 | +23 05 43.832242337 | 8.14 | 6.29 | 4.63 | 3.07 | 1.76 | M3IIb: | 113 | 0 |
15 | * nu. Vir | LP* | 11 45 51.5595979999 | +06 31 45.748996439 | 7.32 | 5.54 | 4.04 | 2.79 | 1.78 | M1III | 259 | 0 |
16 | PN Sa 3-22 | Sy* | 13 14 30.3005092416 | -58 51 49.628844504 | 13.91 | 12.06 | M4.5III | 22 | 1 | |||
17 | V* V840 Cen | Sy* | 13 20 49.4620989744 | -55 50 14.558685540 | 12.951 | K5IIIe | 19 | 0 | ||||
18 | WRAY 15-1108 | Sy* | 13 30 37.1497862472 | -57 58 20.207764416 | 12.5 | M3 | 18 | 0 | ||||
19 | V* V744 Cen | LP* | 13 39 59.8072612685 | -49 56 59.855085294 | 8.65 | 7.50 | 6.00 | M6III | 77 | 0 | ||
20 | * m Vir | PM* | 13 41 36.7700844816 | -08 42 10.729027692 | 8.59 | 6.64 | 5.01 | M1+III | 109 | 0 | ||
21 | * 87 Vir | PM* | 13 47 25.3912914624 | -17 51 35.418569076 | 8.99 | 7.05 | 5.43 | M2III | 72 | 0 | ||
22 | V* ER Vir | LP* | 14 06 41.6449834896 | -14 12 17.597713140 | 8.16 | 6.61 | M4III | 42 | 0 | |||
23 | V* ET Vir | LP* | 14 10 50.4870574246 | -16 18 07.310535267 | 8.76 | 6.63 | 4.91 | M2IIIa | 98 | 0 | ||
24 | BD-21 3873 | Sy* | 14 16 34.2914973552 | -21 45 50.036218344 | 12.060 | 10.684 | K2e | 81 | 0 | |||
25 | V* V768 Cen | LP* | 14 48 38.0463379536 | -36 38 04.908691464 | 7.37 | 6.01 | M5III | 35 | 0 | |||
26 | V* AG Dra | Sy* | 16 01 41.0120557968 | +66 48 10.135056672 | 11.50 | 11.06 | 9.74 | 8.52 | K3IIIep | 501 | 0 | |
27 | WRAY 15-1511 | Sy* | 16 35 15.0820930416 | -51 42 27.579159756 | 14.14 | 13.92 | 12.78 | 11.47 | 9.80 | M2e | 36 | 0 |
28 | Hen 3-1341 | Sy* | 17 08 36.5710647672 | -17 26 30.408149004 | M3.5 | 60 | 0 | |||||
29 | V* RS Oph | Sy* | 17 50 13.1591484960 | -06 42 28.480729788 | 11.884 | 10.776 | 11.228 | K5.5/M0IIIe | 1090 | 0 | ||
30 | * 104 Her | V* | 18 11 54.1566238248 | +31 24 19.256317416 | 8.56 | 6.62 | 4.97 | M3III | 121 | 0 | ||
31 | * 106 Her | PM* | 18 20 17.9149366104 | +21 57 40.667073804 | 8.54 | 6.54 | 4.96 | 3.62 | 2.62 | M1III | 98 | 0 |
32 | WRAY 15-1864 | Sy* | 18 20 19.0481929688 | -26 22 46.224543227 | 12.5 | 14.50 | M5 | 24 | 0 | |||
33 | V* V1743 Cyg | LP* | 19 33 41.6060468328 | +49 15 44.347514508 | 9.37 | 7.60 | 5.96 | M4.5III | 79 | 0 | ||
34 | V* NU Pav | LP* | 20 01 44.7445781273 | -59 22 33.226695613 | 7.97 | 6.66 | 5.13 | M6III | 67 | 0 | ||
35 | * c Sgr | LP* | 20 02 39.4805073281 | -27 42 35.439647267 | 8.03 | 6.23 | 4.58 | 2.71 | 1.15 | M4.5III | 73 | 0 |
36 | V* AG Peg | Sy* | 21 51 01.9739297352 | +12 37 32.127939336 | 9.85 | 8.69 | M3IIIe | 511 | 0 | |||
37 | * ups PsA | * | 22 08 25.9315263653 | -34 02 37.826070169 | 8.28 | 6.47 | 4.99 | K4III | 41 | 0 | ||
38 | * del02 Gru | LP? | 22 29 45.4331493366 | -43 44 57.187958530 | 7.38 | 5.68 | 4.11 | 2.38 | 0.79 | M4.5IIIa | 76 | 0 |
39 | * bet Gru | LP? | 22 42 40.05027 | -46 53 04.4752 | 5.33 | 3.73 | 2.11 | 0.20 | -1.57 | M4.5III | 202 | 1 |
40 | * mu. Peg | PM* | 22 50 00.1930748087 | +24 36 05.692620534 | 5.10 | 4.42 | 3.48 | 2.80 | 2.33 | G8+III | 295 | 0 |
41 | * 55 Peg | V* | 23 07 00.2607332832 | +09 24 34.173822996 | 8.020 | 6.080 | 4.520 | 3.25 | 2.23 | M1IIIab | 142 | 0 |
42 | * phi Aqr | SB* | 23 14 19.3582404192 | -06 02 56.423128812 | 7.64 | 5.77 | 4.22 | 2.94 | 1.86 | M1.5III | 131 | 0 |
43 | * 8 And | V* | 23 17 44.6472657024 | +49 00 55.082930904 | 8.50 | 6.53 | 4.86 | 3.40 | 2.14 | M2.5IIIBa0.5 | 111 | 0 |
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