MOTS EN ANGLAIS EN RAPPORT AVEC «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
TENDANCES D'USAGE DU TERME «X-RAY STAR»
Le terme «X-ray star» est très peu utilisé et occupe la place
167.828 de notre liste de termes les plus utilisés du
dictionnaire anglais.
FRÉQUENCE
Rarement utilisé
Sur la carte précédente est reflétée la fréquence d'utilisation du terme «X-ray star» dans les différents pays.
Tendances de recherche principales et usages générales de
X-ray star
Liste des principales recherches réalisées par les utilisateurs pour accéder à notre
dictionnaire anglais en ligne et des expressions les plus utilisées avec le mot «X-ray star».
10 LIVRES EN ANGLAIS EN RAPPORT AVEC «X-RAY STAR»
Découvrez l'usage de
X-ray star dans la sélection bibliographique suivante. Des livres en rapport avec
X-ray star et de courts extraits de ceux-ci pour replacer dans son contexte son utilisation littéraire.
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
