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| Query : 2002MNRAS.331.1053O |
2002MNRAS.331.1053O - Mon. Not. R. Astron. Soc., 331, 1053-1064 (2002/April-3)
A non-linear theory of vertical resonances in accretion discs.
OGILVIE G.I.
Abstract (from CDS):
In this paper I develop a general theory of vertical resonances, allowing for non-linearity of the response, and dissipation by radiative damping and turbulent viscosity. The problem is reduced to a universal, non-linear ordinary differential equation with two real parameters. Solutions of the complex non-linear Airy equation are presented to illustrate the non-linear saturation of the resonance and the effects of dissipation. It is argued that the m =2 inner vertical resonance is unlikely to truncate the disc in cataclysmic variable stars, but contributes to angular momentum transport and produces a potentially observable non-axisymmetric structure.
Abstract Copyright: 2002 Blackwell Science Ltd
Journal keyword(s): accretion, accretion discs - hydrodynamics - waves - celestial mechanics - binaries: close
Simbad objects: 1
| Number of rows : 1 |
| 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* IP Peg | CV* | 23 23 08.5362249504 | +18 24 59.206884012 | M2 | 395 | 0 |
| Query : 2002MNRAS.331.1053O |
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| SV* SVS 2549 | SBC9 1442 | WEB 20444 | AAVSO 2318+17 |
| LAMOST J232308.57+182459.8 | TIC 243129676 | ZTF17aabulaf |
Gaia DR3 2824150286583562496
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2MASS J23230854+1824593
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V* IP Peg
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EQ 2320+181 |
Gaia DR2 2824150286583562496
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References (395 between 1850 and 2026) (Total 395)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
Link by name to the catalogue in VizieR :
| 2MASS J23230854+1824593 | V* IP Peg | Gaia DR3 2824150286583562496 | Gaia DR2 2824150286583562496 |
Search by coordinates in Vizier (radius: 5 arcsec)
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