Combining this tiny displacement with the hole's previously determined
velocity along the line of sight as it zooms toward Earth yielded its velocity in three dimensions.
Based on the extreme, deduced photometric redshift of GRB 000131 indicating that the gamma rays had travelled an extreme long cosmological distance, astronomers predicted a «break» in the red region of the spectrum around 670 to 700 nm from the strong absorption of light from intervening intergalactic hydrogen
clouds along the line of sight between GRB 000131 and the Solar System.
If instead the distance is about 1,500 light - years (the current best estimate), the long - term dimming could perhaps be because of chance patterns of intervening
dust along the line of sight.
It differs dramatically from the way typical cameras and microscopes focus, which involves moving separate glass lenses back and
forth along the line of sight.
«This means that light from a cosmologically distant quasar will be deflected, or gravitationally lensed, by the intervening
galaxy along the line of sight before arriving at an observer on the Earth,» said Chen of the phenomenon of gravitational lensing, which was predicted by Einstein in 1936.
It could be that the dust and gas exist in a very thin ring sprawled wide around the star, so that the ring blocks
starlight along our line of sight without producing much infrared excess.
Thus, measuring how much gamma rays of different energies are attenuated or weakened from blazars at different distances from Earth indirectly gives a measurement of how many EBL photons of different wavelengths
exist along the line of sight from blazar to Earth over those different distances.
For the transit method to work, a planet must pass almost
perfectly along our line of sight, the chances of which are around 0.5 percent for an Earth - sized planet (in an Earth - sized orbit) and 10 percent for a Jupiter - sized planet (if it orbits near its star)[source: Ames Research Center, FAQ].
For a smaller subset of ten stars, chosen among those with the smallest errors, the astronomers could also retrieve from the literature an estimate of the radial velocity, which quantifies the stellar
motion along the line of sight.
The cylindrically curved crystal provided only a single line of sight through the donut - shaped plasma and could record only the temperature of ions found at
points along that line of sight.
It should be noted that we can measure the movement
only along the line of sight and it is impossible to measure the movement perpendicular to the line of sight.
One must consider the various effects that alter the measured polarized signal, such as the shape of dust grains, the efficiency of grain alignment, the magnetic field properties, and the projection of the
signal along the line of sight.
Messier object number 24 is not a «true» deep sky object, but a huge star cloud in Milky Way, a pseudo-cluster of stars spread thousands of light
years along the line of sight, perceived through a chance tunnel in the interstellar dust.
A carbon monoxide spectrum obtained with HARP in the direction of the Galactic Centre showing the presence of three cold clouds with small line widths and one warmer cloud with larger line width, which move at different
velocities along the line of sight.
Follow - up observations may be able to spot planetary transits, but only if the planets» orbits carry them past their respective
stars along our line of sight.
Our results show not only the magnetic field orientation of around young stellar objects but also the structure of circumstellar matter such as outflow regions and their parent molecular
cloud along the line of sight.
If we live in an infinite universe containing an infinite number of stars, he reasoned, then we should see a star
along all lines of sight.
We need a lens: another galaxy, a heavy one, which can be far away from the source but must sit directly in front of
it along our line of sight.
With enough good quasar spectra, close enough together, the position of the gas clouds can be mapped in three dimensions —
both along the line of sight for each quasar and transversely among dense patches revealed by other quasar spectra.
The spectra revealed each star's velocity
along our line of sight, because a star moving towards us shows a blue shift in its spectrum, whereas a star moving away from us shows a red shift.
A team of astronomers led by Stephan Geier (European Southern Observatory, Garching) observed the known high - velocity star know as US 708 with the Echellette Spectrograph and Imager instrument on the 10 - meter, Keck II telescope to measure its distance and velocity
along our line of sight.
Nine out of ten sources show absorption from H2O + in a range of environments: the molecular clumps surrounding the forming and newly formed massive stars, bright high - velocity outflows associated with the massive protostars, and unrelated low - density clouds
along the line of sight.