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During her time at the University of Washington, she made fundamental contributions to the understanding of stellar binaries, stellar temperatures, chromospheric activity, rotation, and convection.
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With Arthur Milne, a comrade during the war, he wrote a seminal work on stellar spectra, temperatures, and pressures.
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The spectral type is not a numerical quantity, but the sequence of spectral types is a monotonic series that reflects the stellar surface temperature.
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The computed models of observed changes in molecular lines showed that the existence of AGB stars' superwind cannot be explained by the stellar effective temperature.
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In stellar interiors the temperatures are very high.
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It will be fusing hydrogen, at stellar-core pressure and temperature.
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This simple method is conceptually correct, but it cannot be used to obtain stellar temperatures accurately, because stars are not perfect blackbodies. The presence of various elements in the star 's atmosphere will cause certain wavelengths of light to be absorbed. Because these absorption lines are not uniformly distributed over the spectrum, they can skew the position of the spectral peak. Moreover, obtaining a usable spectrum of a star is a time-intensive process and is prohibitively inefficient for large samples of stars
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Observations of NGC 6543 at far-infrared wavelengths (about 60 μm) reveal the presence of stellar dust at low temperatures.
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Stellar models predict a temperature of 15 MK in the center of the Sun, and at the cores of supergiant stars the temperature may exceed 1 GK.
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The triple-alpha steps are strongly dependent on the temperature and density of the stellar material.
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The Hertzsprung–Russell diagram, abbreviated as H–R diagram, HR diagram or HRD, is a scatter plot of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their stellar classifications or effective temperatures.
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Using the stellar spectrum, astronomers can also determine the surface temperature, surface gravity, metallicity and rotational velocity of a star.
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This strong temperature dependence has consequences for the late stage of stellar evolution, the red giant stage.
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Stellar temperatures can be classified by using Wien's displacement law; but this poses difficulties for distant stars.
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Their temperatures measurements of nearby giant stars led to some of the first determinations of stellar diameters.
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The Gamow factor was used in the decade that followed by Atkinson and Houtermans and later by Gamow himself and Edward Teller to derive the rate at which nuclear reactions would proceed at the high temperatures believed to exist in stellar interiors.
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The team used the European Southern Observatory's (ESO's) Very Large Telescope to measure the temperature of the gas right behind the shock wave produced by the stellar explosion.
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Understanding the properties of these dim stellar corpses requires confronting observations with fundamental physics in density and temperature conditions not reproducible in ground-based laboratories. The 'Probing models of pulsars through multi wavelength observations' (PROMOPS) project gathered crucial information on mechanisms of light emission.
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The spectral type is not a numerical quantity, but the sequence of spectral types is a monotonic series that reflects the stellar surface temperature.
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Her thesis research was among the first works to constrain this parameter consistently with the other stellar properties (effective temperature, gravity, etc.).
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A Class B stellar engine is a Dyson sphere—of whichever variant—built around the star, which uses the difference in temperature between the star and the interstellar medium to extract usable energy from the system, possibly using heat engines or photovoltaic cells.
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Using the measured stellar luminosity of Gliese 581 is of 0.013 times that of our Sun, it is possible to calculate Gliese 581c's effective temperature a.k.a. black body temperature. (note: this probably differs from its surface temperature).
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I calculated its abundance of heavy elements and its temperature with stellar spectroscopy.
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What is causing the very high temperatures of stellar coronae, making them visible in X-rays?
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Be stars are generally thought to feature unusually strong stellar winds, high surface temperatures, and significant attrition of stellar mass as the objects rotate at a curiously rapid rate.
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88 sinne gevind in 12 ms. Hulle kom uit baie bronne en word nie nagegaan nie.