Overstable convective modes in rotating early-type stars

نویسندگان

چکیده

We calculate overstable convective (OsC) modes of $2M_\odot$, $4M_\odot$, and $20M_\odot$ main sequence stars. To compute non-adiabatic OsC in the core, we assume $(\nabla\cdot\vec{F}_C)^\prime=0$ as a prescription for approximation called frozen-in convection pulsating stars where $\vec{F}_C$ is energy flux prime $^\prime$ indicates Eulerian perturbation. find that general properties are roughly same those obtained by Lee \& Saio (2020) who assumed $\delta (\nabla\cdot\vec{F}_C)=0$, except no behave like inertial when they tend toward complete stabilization with increasing rotation frequency $\delta$ Lagrangian As increases, stabilized to resonantly excite $g$-modes envelope core rotates slightly faster than envelope. The approximately given $\sigma\sim |m\Omega_c|$ frame hence $\sigma_{m=-2}\approx2\sigma_{m=-1}$ $m$ azimuthal wavenumber $\Omega_c$ core. modal do not strongly depend on mass discuss angular momentum transport resonance suggest transfer takes place from may help rotate uniformly keep low during their evolution

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Normal Modes of Rotating Magnetic Stars

We investigate the effect of a magnetic field on the global oscillation modes of a rotating fluid star in the magnetohydrodynamic approximation. We present general equations for the modification of any type of fluid mode due to a general magnetic field which is not aligned with the star’s spin axis. In the case of any internal dipole magnetic field we derive the equations for the frequency corr...

متن کامل

Inertial modes of slowly rotating isentropic stars

We investigate inertial mode oscillations of slowly and uniformly rotating, isentropic, Newtonian stars. Inertial mode oscillations are induced by the Coriolis force due to the star’s rotation, and their characteristic frequencies are comparable with the rotation frequency Ω of the star. So called r-mode oscillations form a sub-class of the inertial modes. In this paper, we use the term “r-mode...

متن کامل

Surface trapping and leakage of low-frequency g-modes in rotating early-type stars – I. Qualitative analysis

A qualitative study of the surface trapping of low-frequency non-radial g-modes in rotating early-type stars is undertaken within the Cowling, adiabatic and traditional approximations. A dispersion relation describing the local character of waves in a rotating star is derived; this dispersion relation is then used to construct propagation diagrams for a 7M⊙ stellar model, which show the locatio...

متن کامل

Surface trapping and leakage of low-frequency g modes in rotating early-type stars ± II. Global analysis

AB S TRACT A global analysis of the surface trapping of low-frequency non-radial g modes in rotating early-type stars is undertaken within the Cowling, adiabatic and traditional approximations. The dimensionless pulsation equations governing these modes are reviewed, and the boundary conditions necessary for solution of the equations are considered; in particular, an outer mechanical boundary c...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2021

ISSN: ['0035-8711', '1365-8711', '1365-2966']

DOI: https://doi.org/10.1093/mnras/stab1433