QUÉ SIGNIFICA SEMIDETACHED BINARY EN INGLÉS
Estrella binaria
Una estrella binaria es un sistema estelar que consta de dos estrellas que orbitan alrededor de su centro de masa común. La estrella más masiva se llama la primaria y la otra es su estrella compañera, viene / koʊmiːz /, o secundaria. Los sistemas de dos, tres, cuatro o incluso más estrellas se llaman sistemas de estrellas múltiples. Estos sistemas, especialmente cuando están más distantes, a menudo aparecen a simple vista como un único punto de luz, y luego son revelados como dobles por otros medios. La investigación en los últimos dos siglos sugiere que la mitad o más de las estrellas visibles son parte de sistemas estelares múltiples. El término estrella doble es a menudo utilizado sinónimo de estrella binaria; Sin embargo, la estrella doble también puede significar doble estrella óptica. Los dobles ópticos se llaman así porque las dos estrellas aparecen cerca juntas en el cielo como visto de la tierra; Están casi en la misma línea de visión. Sin embargo, su "duplicidad" sólo depende de este efecto óptico; Las estrellas mismas están distantes unas de otras y no comparten ninguna conexión física. Una estrella doble puede ser revelada como óptica por medio de diferencias en sus mediciones de paralaje, movimientos apropiados, o velocidades radiales.
definición de semidetached binary en el diccionario inglés
La definición de binario semiaisplazado en el diccionario es un par de estrellas que están tan juntas que la transferencia de masa ocurre de una a otra.
PALABRAS DEL INGLÉS RELACIONADAS CON «SEMIDETACHED BINARY»
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10 LIBROS DEL INGLÉS RELACIONADOS CON «SEMIDETACHED BINARY»
Descubre el uso de
semidetached binary en la siguiente selección bibliográfica. Libros relacionados con
semidetached binary y pequeños extractos de los mismos para contextualizar su uso en la literatura.
1
The Physical Universe: An Introduction to Astronomy
BOX 10.3 Semidetached Binaries The appearance of a semidetached binary in
which mass is transferred from a normal lobe-filling star to its companion
depends largely on the physical nature of the detached companion. (1) If the
detached ...
2
An Introduction to Close
Binary Stars
The mass ratio (secondary/primary) is q = 0.85. Orbit sizes for detached binaries
range from about 1 Ro up to those of resolved binaries (astronomical units, AUs).
Fig. 1.4. A semidetached binary system, with a mass ratio. 7.5 Types of binaries: ...
3
Zdenek Kopal's
Binary Star Legacy
For these three systems we obtained near-contact configurations, but it is also
possible that BL And might be a semidetached binary. Configuration ofCNAnd is
most probably either detached or semidetached, but our solutions are not
finished ...
Horst Drechsel, Miloslav Zejda,
2005
(b) A semidetached binary occurs when one member star swells up to fill or
overflow its Roche lobe. Gas can then escape from its distorted surface and flow
over to its neighbor, (c) A contact binary consists of two stars, both of which have
filled ...
5
100 Billion Suns: The Birth, Life, and Death of the Stars
Figure 9.2 (a) A detached binary. Both stars are clearly located within the
maximal permitted volume outlined by the broken curved line, (b) A
semidetached binary. The left star completely fills out its Roche volume. one just
about fills its volume ...
6
Relativistic Gravitation and Gravitational Radiation ...
Semidetached binary evolution We consider a compact (primary) star of mass MI
in an orbit of separation a with a non-compact secondary of mass MI- In all cases
of interest, tidal dissipation in the latter star keeps the binary orbit circular and ...
Jean-Alain Marck, Jean-Pierre Lasota,
1997
7
A Dictionary of Astronomy
The variable period and the emission lines that are sometimes detectable in its
spectrum are evidence for *mass transfer, indicating that the system is a *
semidetached binary. The eclipsing pair, which consists of a B8 dwarf and a K2
subgiant, ...
8
Evolutionary Processes in Interacting
Binary Stars
... it had become a semidetached binary, after RLOF. In a semi-detached binary
undergoing conservative case D mass transfer, after passing the critical mass
ratio (defined later), the loser would lose mass on its nuclear timescale. Since ...
Y. Kondo, R.F. Sisteró, R.S. Polidan,
1992
9
Binary and Multiple Stars as Tracers of Stellar Evolution: ...
... in fact observed. 289 Z. Kopal and J. Rahe (eds.), Binary and Multiple Stars as
Tracers of Stellar Evolution, 289-299. Copyright © 1982 by D. Reidel Publishing
Company. 2. Evolution from a detached or semidetached binary by angular XLIII.
International Astronomical Union. Colloquium, Z. KOPAL (Ed), Jürgen Rahe,
1982
10
Advances in Stellar Evolution
The model space densities of wide, close detached, and semidetached binary
degenerates are consistent with observations. Recent studies by Marsh and his
collaborators have significantly increased the number of known detached close ...
Robert T. Rood, Alvio Renzini,
1997