Exact(5)
Because planets form within the whirling disk of gas and dust that extends out from a rotating star, they ought to have orbits that follow the star's rotation.
Pulsar radiation is polarized, both linearly and circularly, and can be understood in terms of a rotating star having a powerful magnetic field of a trillion gauss.
We performed 2D and full 3D magnetohydrodynamic simulations of disk accretion to a rotating star with an aligned or misaligned dipole magnetic field.
The eclipsing exoplanet allows astronomers to rely on the Doppler shift phenomenon that creates subtle color changes measured by a high resolution spectograph when something moves, such as a rotating star.
But a rotating star is not spherical in shape, it has an equatorial bulge.
Similar(55)
I will present global relativistic simulations of the interaction between a rotating stars magnetic field and an accretion disk, showing the opening of field lines, the formation and reconnection of current sheets, and a large increase in the spin-down torque applied by the pulsar wind.
In this article, we describe the ESTER code, which is the first code able to compute in a consistent way a two-dimensional model of a fast rotating star including its large-scale flows.
Schematic profiles of the midplane angular velocity of the plasma for the case of a slowly rotating star (left-hand panel) and a rapidly rotating star (right-hand panel) which is in the propeller regime.
Collimation and driving of the outflows Figure 3 shows the long-distance development of a conical wind from a slowly rotating star.
It was also confirmed that GJ 3634 is neither a binary star nor a quickly rotating star, common false positives when searching for transiting planets.
However, this discrepancy can be explained if Vega is a rapidly rotating star that is being viewed from the direction of its pole of rotation.
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