PALABRAS DEL INGLÉS RELACIONADAS CON «X-RAY STAR»
X-ray star
cindy
star
mortgage
fired
merriam
webster
luminous
celestial
object
emitting
major
portion
radiation
form
rays
called
also
source
first
known
stuff
nasa
science
astronomers
using
chandra
observatory
seeing
supernovae
spray
essential
elements
life
into
interstellar
space
binary
stars
imagine
universe
this
site
intended
students
anyone
interested
learning
about
translations
information
encyclopedia
reference
usually
that
strong
emitter
cygnus
more
yourdictionary
starlike
nova
pulsar
noun
especially
emits
unusually
camp
joseph
julian
soria
joins
family
film
boaz
yakin
directing
movie
which
josh
wiggins
thomas
haden
dutch
dict
german
collins
always
spanish
italian
TENDENCIAS DE USO ACTUALES DEL TÉRMINO «X-RAY STAR»
El término «X-ray star» se utiliza muy poco y ocupa la posición
167.828 de nuestra lista de términos más usados del
diccionario de inglés.
FRECUENCIA
Raramente usado
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Principales tendencias de búsqueda y usos comunes de
X-ray star
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10 LIBROS DEL INGLÉS RELACIONADOS CON «X-RAY STAR»
Descubre el uso de
X-ray star en la siguiente selección bibliográfica. Libros relacionados con
X-ray star y pequeños extractos de los mismos para contextualizar su uso en la literatura.
You are an x-ray star That's what you are Shining from afar So here you roar You
are an x-ray star My hot red sports car My light in the dark All what I live for You
are an x-ray star You raise the bar More thanjust par My genie in ajar You are my
...
2
The Handy Astronomy Answer Book
As a percentage of the total radiation emitted by the Sun, however, its an X-ray
star's emission is very small. Xray stars may emit thousands of times more X-rays
than visible light radiation. X-ray stars are almost always binary star systems or ...
4686 emission originates near but not at the X-ray star. The entire Roche lobe of
the X-ray star may be filled by an accretion disk. The existence of a disk was
evidenced by analyses of the optical tvan Paradijs and Zuiderwijk 1977i and UV
lvan ...
Bengt E. Westerlund, 1997
M% and Mv are masses of the X-ray star and the visible star respectively, AT, and
ATV are the orbital velocities of the two stars and i is the orbital inclination. From
a knowledge of r, sin i and P^, one determines/Cm). Ratio of masses q is ...
[258] analyzed the optical light curve, deduced a conservative lower limit of MX >
2.8M0, and concluded that the X-ray star is likely a black hole. Thus, LMC X-3 is a
strong BHC; however, the possibility of it being a massive neutron star primary ...
Walter H. Lewin, Walter H. G. Lewin, Jan van Paradijs, 1997
6
The Evolving Universe and the Origin of Life: The Search for ...
However, the x-ray star shows no signs of pulsing which could be related to a
rotating neutron star. Studies of the binary motion have shown that the x-ray star
consists of at least 5 solar masses of matter; it can be even ten times heavier than
...
Pekka Teerikorpi, Mauri Valtonen, K. Lehto, 2008
7
Suzaku Studies of White Dwarf Stars and the Galactic
X-
ray ...
... (<50 %), star forming galaxies ('2), and cosmological shocks ('2) aTypical
wavelength/energy ranges in which the background emission is observed
synthesizing the GRXE spectrum using those of known X-ray star populations in
the Galaxy.
8
Black Hole Astrophysics: The Engine Paradigm
In both cases the X-rays are produced when matter is accreted from the
companion onto the X-ray star. However, in the LMXB case it is due exclusively to
“Roche lobe overflow” (Fig. 3.5a). This occurs when the companion star expands
and ...
9
The World Book Dictionary
X-ray source, = X-ray star. X-ray spectrometer, a spectrometer using X rays by
which the chemical constituents of a substance are separated into their
characteristic spectral lines for identification and determination of their
concentration.
10
Exploring the
X-
ray Universe
They represented the standard X-ray star and accounted for many of the
remarkable properties which attracted attention after the discovery of Sco X- 1 .
The important point is that the enormous gravitational potential of neutron stars
and black ...
Philip A. Charles, Frederick D. Seward, 1995