2002MNRAS.331.1053O


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):

An important and widely neglected aspect of the interaction between an accretion disc and a massive companion with a coplanar orbit is the vertical component of the tidal force. As shown by Lubow, the response of the disc to vertical forcing is resonant at certain radii, at which a localized torque is exerted, and from which a compressive wave (p mode) may be emitted. Although these vertical resonances are weaker than the corresponding Lindblad resonances, the m =2 inner vertical resonance in a binary star is typically located within the tidal truncation radius of a circumstellar disc.

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

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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

Basic data :
V* IP Peg -- Cataclysmic Binary
Other object types:
otypes_help
CV* (2020MNRAS), V* (V*,AAVSO), * (WEB,Gaia), SB* (SBC9), PM* (2018yCat), NIR (2MASS), Opt (LAMOST), ev (ZTF)
ICRS coord. (ep=J2000) :
23 23 08.5362249504 +18 24 59.206884012 (Optical) [ 0.0290 0.0229 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
23 20 38.6391258112 +18 08 32.516738770 [ 0.0290 0.0229 90 ]
Gal coord. (ep=J2000) :
095.3338874816037 -39.6768881367989 [ 0.0290 0.0229 90 ]
Proper motions mas/yr :
-61.849 -33.309 [0.040 0.028 90] A 2020yCat.1350....0G
Parallaxes (mas):
7.093 [0.0377] A 2020yCat.1350....0G
Spectral type:
M2 D ~
Fluxes (4) :
G 14.672627 [0.016719] C 2020yCat.1350....0G
J 12.601 [0.024] C 2003yCat.2246....0C
H 11.975 [0.022] C 2003yCat.2246....0C
K 11.721 [0.020] C 2003yCat.2246....0C
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Identifiers (12) :
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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
2MASS J23230854+1824593 V* IP Peg EQ 2320+181 Gaia DR2 2824150286583562496

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).
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Collections of Measurements Description of Measurements

Distance : 3    Var : 3    Plx : 2    PM : 2   

   

Observing logs
IUE : 32   

   


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2MASS J23230854+1824593 V* IP Peg Gaia DR3 2824150286583562496 Gaia DR2 2824150286583562496

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