23 Übersetzungen
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- However, there is little central concentration of the X-ray emission.
- It has a relatively long period and low eccentricity for this type of binary, which means the x-ray emission is persistent and not usually strongly variable.
- He would have seen x-ray emission lines for both elements, but assumed that the dominant ones belonged to holmium, instead of the dysprosium impurity.
- Observations performed by Stefanie Komossa and collaborators with the Chandra X-Ray Observatory have detected strong hard X-ray emission from both of the nuclei.
- The source for this strong X-ray emission is Epsilon Eridani's hot corona.
- One of the great surprises of Hyakutake's passage through the inner Solar System was the discovery that it was emitting X-rays, with observations made using the "ROSAT" satellite revealing very strong X-ray emission.
- The variations in temperature are often correlated with changes in the X-ray emission.
- This type of biomonitoring has been achieved with newer microanalytical techniques like synchrotron radiation based X-ray fluorescence spectroscopy and microparticle induced X-ray emission.
- X-ray emission is expected from astronomical objects that contain extremely hot gases at temperatures from about a million kelvin (K) to hundreds of millions of kelvin (MK).
- X-ray observations have proven useful for studying young stars, since X-ray emission from these objects is about 100–100,000 times stronger than X-ray emission from main-sequence stars.
- The model also shows that X-ray emission from ejecta heated up by the shock will be dominant very soon, after which the ring would fade away.
- Consuming 75% of production, the primary use for strontium was in glass for colour television cathode-ray tubes, where it prevented X-ray emission.
- Attempts to detect X-ray emission from Procyon with nonimaging, soft X-ray-sensitive detectors prior to 1975 failed.
- Although much of the optical and X-ray emission from supernova remnants originates from ionized gas, a great amount of the radio emission is a form of non-thermal emission called synchrotron emission.
- Observation of X-ray emissions allows astronomers to study celestial phenomena involving gas with temperatures in the millions of degrees.
- In 1969 Donald Lynden-Bell proposed that nearby galaxies contain supermassive black holes at their centers as relics of "dead" quasars, and that black hole accretion was the power source for the non-stellar emission in nearby Seyfert galaxies.
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