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Luminosity issues for the ee
Luminosity is an important parameter when deriving cross
Luminosity is not calculated
Luminosity is compared with the ``measured" Luminosity where various detector angular resolutions and polar angle coverages are
Luminosity is from helsdon & ponman
Luminosity is a measure of particle interaction
Luminosity is “sound and well
Luminosity is measured relative to
Luminosity is measured usually in cm^
Luminosity is set to 100% diffuse is set to 100%
Luminosity is also related to a star's size
Luminosity is based upon our best estimate of the collider Luminosity
Luminosity is not isotropic
Luminosity is the total amount of energy produced in a star and radiated into space in the form of em radiation
Luminosity is a measure of the intrinsic brightness of a light source
Luminosity is high
Luminosity is global analysis
Luminosity is used as a sfr tracer for objects with redshift larger than 0
Luminosity is quite different
Luminosity is nul
Luminosity is approached
Luminosity is a measure of power divided into units called watts
Luminosity is only 45% of our sun’s Luminosity
Luminosity is watts
Luminosity is such a strong function of the mass of the star has great implications for how long stars live on the main sequence
Luminosity is significantly reduced and is
Luminosity is reduced from the geometrical
Luminosity is related to its mass
Luminosity is an intrinsic property of a star
Luminosity is an important one
Luminosity is red close to the object and passes through yellow to green and possibly blue as distance from the surface of
Luminosity is not efficient
Luminosity is controlled by the
Luminosity is determined with a different detector
Luminosity is directly related to the observed flux without the extra complication of uncertain
Luminosity is underestimated by about 200 ipb
Luminosity is higher
Luminosity is reopened
Luminosity is the power radiated by an object
Luminosity is independent of period
Luminosity is predominantly due to the binaries consisting of an accreting ns with a giant or supergiant companion which does not fill its
Luminosity is conserved to within 3 percent at every radial grid point
Luminosity is the amount of energy a body radiates in unit time
Luminosity is 4
Luminosity is described by a power
Luminosity is adequately sampled
Luminosity is directly dependent upon its mass
Luminosity is declared
Luminosity is about half of that for the liquid
Luminosity is the
Luminosity is not very sensitive to the cutoff
Luminosity is proportional to 1/
Luminosity is simply that
Luminosity is proportional to
Luminosity is expected as the bunch intensities are increased
Luminosity is obtained for ie
Luminosity is very easily determined from total energy
Luminosity is proportional to mass n
Luminosity is 1/3 solar
Luminosity is the average over the last few weeks during which the Luminosity was fairly constant
Luminosity is the accretion process itself
Luminosity is proportional to 1/r2
Luminosity is
Luminosity is the amount of light energy emitted by the star within a second
Luminosity is 100
Luminosity is attenuated by two factors
Luminosity is lost
Luminosity is 4 × 10 33 ergs per second
Luminosity is open for
Luminosity is a number describing the intensity of a particle beam and is measured in cm
Luminosity is a measure of the 'light
Luminosity is defined as the proportionality constant between the proton
Luminosity is not available in most scanning programs and is available with some inconvenience in photoshop
Luminosity is found to be negligible compared to the disk's Luminosity
Luminosity is known
Luminosity is estimated in section 3
Luminosity is proportional to radius x temperature
Luminosity is lower than at their early young age
Luminosity is limited and therefore only effective when the pomeron
Luminosity is extremely high
Luminosity is averaged over 5 hours due to the beam
Luminosity is 2*10^32; to change it you need a complete dbase copy that you use as your default database;
Luminosity is about 50
Luminosity is measured by detection of the bremsstrahlung process
Luminosity is achieved by merely pushing the contrasts until the light dominates everything
Luminosity is energy emitted per unit time * the Luminosity of a blackbody
Luminosity is dependent on black hole mass and accretion rate