Results 241 to 250 of about 3,161,922 (291)

High-performance temperature regulation of nonlinear CSTRs via a hybrid stellar oscillation optimizer and differential evolution-based PID-F control. [PDF]

Sci Rep
Ekinci S, Turkeri C, Gokalp I, Li Y, Li D.   +4 more
europepmc   +1 more source

Uncovering the rapidly evolving orbits of the dynamic TOI-201 system. [PDF]

Sci Adv
Mireles I, Ulmer-Moll S, Liveoak D, Dragomir D, Korth J, Venner A, Collins KA, Triaud AHMJ, Guillot T, Petit A, Carmichael T, Millholland S, Hallatt T, Parviainen H, Osborn HP, Rapetti D, Baycroft TA, Bhatnagar S, Bouchy F, Dancikova R, Figueira P, Lendl M, Udry S, Wheatley P, Abe L, Agabi A, Beltrame M, Bendjoya P, Deloupy V, Mékarnia D, Schmider FX, Suárez O, Barkaoui K, Horne K, Murgas F, Palle E, Schwarz RP, Sefako R, Shporer A, Srdoc G, Stockdale C, Wilkin FP, Hartman JD, Sgro LA, Tan TG, Jenkins JM, Bódi A, Havell D, Rivett D, Transom I.   +49 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Stellar Structure and Stellar Evolution

Lecture Notes in Physics, 1991
exaly   +2 more sources

Stellar Structure and Evolution

Astronomy and Astrophysics Library, 2012
This long-awaited second edition of the classical textbook on Stellar Structure and Evolution by Kippenhahn and Weigert is a thoroughly revised version of the original text.
Achim Weiss, Rudolf Kippenhahn, Alfred Weigert   +2 more
exaly   +2 more sources

Stellar Evolution

2004
Abstract The physical structures and properties of stars change as they age. In this chapter, we give an overview of the way stars evolve to set the context for our later discussions. The mass is by far the most important single factor determining a star’s structure and evolution.
T W Hartquist, J E Dyson, D P Ruffle
openaire   +2 more sources

Fred’s Contributions to Stellar Evolution

Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire   +2 more sources

Stellar Evolution and Stellar Structures

1995
It is often thought that very little was known about the stars in the nineteenth century because most astronomy books of the time tended to concentrate on the planets. This was far from the truth, however, although nineteenth century knowledge of the stars was purely observational, with no understanding of their internal processes. In fact, at the time
openaire   +1 more source

Stellar Evolution

Transactions of the International Astronomical Union, 1962
It is perhaps one of the most important characteristics of the past decade in astronomy that the evolution of some major classes of astronomical objects has become accessible to detailed research. The theory of the evolution of individual stars has developed into a substantial body of quantitative investigations. The evolution of galaxies, particularly
openaire   +1 more source

Stellar Populations, Stellar Evolution, and Stellar Atmospheres

2021
J. J. Eldridge, E. R. Stanway
openaire   +1 more source