Results 261 to 270 of about 492,459 (298)
Some of the next articles are maybe not open access.
Astrophysics, 1975
In this paper I have set forth in detail the theory of thermal waves in inhomogeneous media; it has, I believe, independent theoretical interest. I wish also to point out the fact that the mechanism of separation of an envelope in a nova explosion has hitherto remained obscure, since it strongly depends on the nature of the energy source of the ...
openaire +1 more source
In this paper I have set forth in detail the theory of thermal waves in inhomogeneous media; it has, I believe, independent theoretical interest. I wish also to point out the fact that the mechanism of separation of an envelope in a nova explosion has hitherto remained obscure, since it strongly depends on the nature of the energy source of the ...
openaire +1 more source
GRAVITATIONAL-WAVE INSTABILITIES IN ROTATING STARS
International Journal of Modern Physics A, 2002This article provides a brief overview of recent research into the gravitational-wave driven instability of the r-modes in rotating neutron stars.
openaire +1 more source
2010
Wave Star is a Wave Energy device developed and installed in Denmark. The paper describes the scale 1:40 model installed in Nissum Bredning in 2006, and gives production figures from this installation. Further the Hanstholm Scale 1:2 model is described.
Frigaard, Peter Ba +3 more
openaire +1 more source
Wave Star is a Wave Energy device developed and installed in Denmark. The paper describes the scale 1:40 model installed in Nissum Bredning in 2006, and gives production figures from this installation. Further the Hanstholm Scale 1:2 model is described.
Frigaard, Peter Ba +3 more
openaire +1 more source
Wave Propagation in Pulsating Stars
Astrophysics and Space Science, 1998Lissajous diagrams are used to detect phase lags between radial velocity curves associated with different ions. Present in many kind of variable stars, this effect provides an important tool to study the atmosphere dynamics.
openaire +1 more source
Wave Star C5:Wave forces on foundation piles
2007Design pile loads in this document are based on the Morison equation. In Chapter 3 and 4 the background for the design loads provided in Chapter 5 are given. In the remaining chapters from Chapter 6 and onward discussions and explanations of the results are given.A historical list of activities up to the present revision is given in Appendix A ...
Kramer, Morten; id_orcid 0000-0002-5810-5564 +1 more
openaire +2 more sources
Astrophysics and Space Science, 1972
It is shown by a certain combination of stella parameters and energy which was released by a outburst, the transfer of that energy outwards is carried out by the thermal wave.
openaire +1 more source
It is shown by a certain combination of stella parameters and energy which was released by a outburst, the transfer of that energy outwards is carried out by the thermal wave.
openaire +1 more source
Wave-Rotation Interaction in Stars
Publications of the Astronomical Society of Japan, 1983Abstract The wave-rotation interaction is formulated in terms of Reynolds stress in rotating stars. How the rotation change is connected with wave dissipation, excitation, and transience is demonstrated in the case of the slowly rotating stars. How the nonaxisymmetric nonradial oscillations can redistribute the angular momentum in stars,
openaire +1 more source
The induced star formation: Combustion waves and star bursts
Astrophysics and Space Science, 1989One of interactions of young active stars with interstellar gas is excitation of shock waves, that compress the gas and favour the formation of new generation of stars. Thus, a positive feedback between stellar and gaseous constituents is realized. When spread from point to point this interaction gives rise to a stationary wave of star formation.
openaire +1 more source
Shock Waves in Outflows from Young Stars
Astrophysics and Space Science, 2003This review focuses on physics of the cooling zones behind radiative shocks and the emission line diagnostics that can be used to infer physical conditions and mass loss rates in jets from young stars. Spatial separations of the cooling zones from the shock fronts, now resolvable with HST, and recent evidence for C-shocks have greatly increased our ...
openaire +1 more source