Starting from the yellow star, the trajectory moves on the slow timescale associated with (na_{i}) along the stable lower branch of S until it reaches the lower fold.
Starting from the yellow star in Fig. 14, the trajectory is in the silent phase and evolves on the slow timescale under the slow reduced layer problem (9a)–(9b), until it approaches sufficiently close to the superslow manifold (mathscr {M}_{ss}) (near the yellow circle).
Starting from the yellow star at low (c_{mathrm{tot}}) and l (Fig. 10), a sequence of small bursts is produced as the trajectory in ((ca_{i}, na_{i}))-space oscillates between the LF and HC curves multiple times (Fig. 10B).
You know how all the matter in the universe started from stars and we are, therefore, stardust?
How to live for ever Reprints Related items Europa's ocean: A lonely sea in the skyAug 24th 2000Dr Turnbull starts from the premise that every star has a zone around it with the right temperature to support carbon-and-water-based life, the only sort so far known to exist.
She contributed to the understanding of the phases of life of low and intermediate mass stars, starting from the first contraction of the forming stars (pre-main-sequence) ending with the latest white dwarf cooling stages.
Awesome Speed, starting from the No. 4 post, and Abiding Star, starting from the No. 9, have both won in Maryland, but neither has shown an ability to beat the elite of this 3-year-old crop.
Abiding Star, which will start from the No. 9 post Saturday, has been "very competitive and seems to be getting a lot better with every start, but he hasn't met the Muhammad Alis of the game as of yet," Allard said.
Jukna [30] determined graph complexity as the minimum number of union and intersection operations required to obtain the whole set of its edges starting from star graphs.
To find k, we follow the arguments of[15, 16]: for a light starting from a certain star with a frequency ν0(τ = 0), then its frequency at time τ is given according to the principle of general relativity by ν τ = ν τ = 0 1 + τ ( d h ^ 00 / dτ Open image in new window. Now for R = τ, we get ν τ = ν τ = 0 1 + R ( d h ^ 00 / dτ Open image in new window.
