「magnitudes」の共起表現(1語右で並び替え)

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deriving	magnitudes accurate to about 0.1 mag; and
e universe was more constant in color across	magnitudes and the blue cloud was not as uniformly dist
Its apparent visual magnitude varies by 0.02	magnitudes and is approximately 7.72 at maximum brightn
logue that tracks proper motions, positions,	magnitudes and other characteristics for over one billi
It contains positions, proper motions,	magnitudes, and spectral types, and was published by th
oids used in crystallography to indicate the	magnitudes and directions of the thermal vibration of a
ose apparent visual magnitude varies by 0.06	magnitudes and is approximately 4.39 at maximum brightn
Their apparent visual	magnitudes are 6.3, 6.2, and 7.4, respectively.
Its components' apparent	magnitudes are 6.51 and 7.81.
	Magnitudes are said to have a ratio to one another whic
Variations in brightness on the order of 0.1	magnitudes are associated with the radial pulsations, w
ys the system decreases in brightness by 1.1	magnitudes as the brighter star is partially eclipsed b
ass of variable stars, which fade by several	magnitudes at irregular intervals.
lis as an irregular variable with a range of	magnitudes between 3.7 and 4.1 and a periodicity of rou
ermining Cepheid Scale Distance and absolute	magnitudes beyond the realm of parallax measurement, on
xample is the star V1057 Cyg, which became 6	magnitudes brighter and went from spectral type dKe to
Note that the dataset is complete for small	magnitudes, but becomes erratic for the larger.
he B-V colour index increases, since smaller	magnitudes correspond to brighter light.
sed on the idea that instants, instantaneous	magnitudes, determined positions, and time itself, do n
The secondary, HIP 12635 is 1.521	magnitudes fainter and located at a separation of 14.6
parition, the comet has always been over two	magnitudes fainter and no fragments have been seen sinc
hite A-type main sequence dwarf, about three	magnitudes fainter than the primary.
since thermal conductivity of water is some	magnitudes higher.
ibrations are usually anisotropic (different	magnitudes in different directions in space), an ellips
lar character of relationship as the one for	magnitudes in chemical kinetics where various predators
(Different sources give apparent	magnitudes in the range 2.99-3.03.)
d brightness variation was approximately 0.3	magnitudes in 1971, by 1980 it was merely 0.1 magnitude
i has been found to vary very slightly (0.02	magnitudes) in brightness.,
ar GSC 3656-1328 suddenly brightened by four	magnitudes in two weeks time and returned to its normal
ound extinction in its direction reaching 24	magnitudes in the visible light.
Although earthquakes with	magnitudes in the 6-7 range are not normally associated
cumulative frequency of each of the observed	magnitudes in a data series of the variable.
luminosity varied ±8% from its average (0.15	magnitudes in total) with a 3.97 day period; however, t
The comparison of the optical and infrared	magnitudes including dust condensation has allowed astr
When comparing	magnitudes, it is often helpful to use a logarithmic sc
act calculation) as well the names, natures,	magnitudes, latitudes, longitudes, aspects, declination
nces can be positive or negative, with their	magnitudes limited by a number representative of the ma
o fuse, with the Autorooper becoming several	magnitudes more powerful and deadly than it originally
Two strong earthquakes with	magnitudes Ms 6.4 and 6.3 occurred on January 21, 1997
il 6, 6, 11, 16, other four earthquakes with	magnitudes Ms 6.3, 6.4, 6.6, 6.3 killed 8 people.
lts may lead to a major underestimate of the	magnitudes of the largest possible earthquake.
1:54 GMT and 4:10 GMT on March 6, 1987 with	magnitudes of 6.1 and 6.9 on the surface wave magnitude
, and is composed of two stars with apparent	magnitudes of +4.4 and +6.5 which are separated by 0.02
main sequence dwarfs and both have apparent	magnitudes of +5.3.
bility; the exact value of E0 depends on the	magnitudes of the dipole matrix elements and on the ene
kcal/mol) was small compared to the absolute	magnitudes of the energies and entropies involved (~100
ostellar core Cha-MMS1 based on the relative	magnitudes of the abundances.
The thesis dealt with colors and	magnitudes of galaxies.
They have apparent	magnitudes of +4.2 and +4.4,
The two components have	magnitudes of +5.3 and +5.4 and are separated by 0.0002
The	magnitudes of such earthquakes are considered to have b
Megathrust quakes have	Magnitudes of 9.5+, but Puerto Rico hasn't even reached
a spectroscopic binary whose components have	magnitudes of +4.1 and +5.6.
They have apparent	magnitudes of +6.18 and +7.00 and are separated by 8 ar
ustal earthquakes of central Greece have had	magnitudes of about 7.2.
te A-type main sequence dwarfs with apparent	magnitudes of 5.2 and 5.5 respectively.
Two	magnitudes of a continuous quantity stand in relation t
The	magnitudes of the Gamma Volantis stars are fourth and s
ten brightest spiral galaxies have apparent	magnitudes of 12-14 that are observable with amateur te
A-type main sequence stars and have apparent	magnitudes of +4.75 and +4.83.
te B-type main sequence dwarfs with apparent	magnitudes of +5.9 and +6.4.
surface brightness is very low, with surface	magnitudes of between +15.99 and +25 reported.
Because of the large	magnitudes of lithostatic stress in tectonic plates, te
ary, and the two subcomponents have apparent	magnitudes of +5.0 and +6.3 and are separated by 0.0047
The axial ratio is the ratio of the	magnitudes of the major and minor axis defined by the e
ely 30 Astronomical Units, and have apparent	magnitudes of +5.8 and +6.2.
and have estimated maximum credible Richter	magnitudes of 8.3 and 7.3 respectively.
ch are 32 arcseconds apart and have apparent	magnitudes of +6.9 and +7.8.
s, attempting to get consistent data for the	magnitudes of the comet nuclei.
The relative	magnitudes of the harmonics of the Earth's tides depend
-2 Tucanae, are 27 arcseconds apart and have	magnitudes of between 4 and 5.
The component stars of ε1 have	magnitudes of 4.7 and 6.2 separated by 2.6" and have an
eriment, one of the few experiments by which	magnitudes of second order in v/c could be detected.
tity is a property that exists in a range of	magnitudes or multitudes.
iable star and its brightness varies by 0.02	magnitudes over periods of 0.5 to 2.4 hours.
, and the binary's brightness varies by 0.12	magnitudes over a period of 1.45 days.
The catalog contains positions,	magnitudes, proper motions and spectral types and has e
Numbers are represented by physical	magnitudes such as may be done with certain rotational
tities but may also entail relations between	magnitudes that can be established through experiments
ast methods for measuring star positions and	magnitudes, thereby making a pioneering work for modern
s of the amount of reddening range from 0.18	magnitudes, to as high as 0.41 magnitudes.
be stated in comparisons between particular	magnitudes, unlike quality which is marked by likeness,
riable star and its brightness varies by 0.2	magnitudes with a period equal to its orbital period of
and typical brightness fluctuations are 0.1	magnitudes with periods on the order of one day.
ariables change in brightness by 0.01 to 0.3	magnitudes with periods of 0.1 to 0.6 days.
Its brightness varies by 0.06	magnitudes with a period equal to its orbital period of
iable star and its brightness varies by 0.56	magnitudes with a period of 119 days.
able star and its brightness varies by 0.015	magnitudes with a period of 2.42 hours.
iable star and its brightness varies by 0.07	magnitudes with a period of a few hours.
iable star and its brightness varies by 0.02	magnitudes with a period of 50.40 minutes.
iable star and its brightness varies by 0.02	magnitudes with a period of 23.57
iable star and its brightness varies by 0.04	magnitudes with a period of 2.61 days.
iable star and its brightness varies by 0.01	magnitudes with a period of 1.61 hours.
iable star and its brightness varies by 0.14	magnitudes with a period of 82.8 days.
all apparent visual magnitude varies by 0.04	magnitudes with a period of 2.344 days, and is approxim
lescope as there are a wide range of stellar	magnitudes within the cluster easily viewed in one smal

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