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| Query : 1999ApJ...518..814M |
1999ApJ...518..814M - Astrophys. J., 518, 814-820 (1999/June-3)
What can the kinematic complexity of astrophysical shear flows lead to?.
MAHAJAN S.M. and ROGAVA A.D.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Hydrodynamics - Instabilities - Waves
Simbad objects: 3
| Number of rows : 3 |
| 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 | V* V1213 Tau | Or* | 04 31 37.5055489536 | +18 12 24.383952396 | K7 | 605 | 0 | |||||
| 2 | M 87 | AGN | 12 30 49.42338414 | +12 23 28.0436859 | 10.16 | 9.59 | 8.63 | 7.49 | ~ | 7815 | 3 | |
| 3 | V* R Aqr | Sy* | 23 43 49.4634303216 | -15 17 04.176349872 | 8.823 | 7.683 | 9.37 | M6.5-8.5e | 823 | 0 |
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