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Showing 1 to 5 of 5 for “"Wolf-Rayet stars"”.

  1. Massive stars in the Galactic Center Quintuplet cluster

    … cluster, the spectral analysis of the cluster Wolf-Rayet stars of the nitrogen sequence to determine their fundamental stellar parameters, and discusses the obtained results in a general context. The Quintuplet cluster was discovered in one of the first infrared surveys of the Galactic center …

    potsdam-diss Repository record for Massive stars in the Galactic Center Quintuplet cluster (opens in a new tab)

  2. Celestial Paleontology: The Legacy of Dying Stars

    <p>In their death throes, stars dole out their atmospheric material to the interstellar medium in dramatic stellar winds and spectacular explosions. The details of this profound metamorphosis, from star to remnant, play a key role in the next generation of star formation as well as the energetic …

    denver Repository record for Celestial Paleontology: The Legacy of Dying Stars (opens in a new tab)

  3. A New Era of Observational Capability at Ritter Observatory: Spectropolarimetry from Exoplanets to Circumstellar Disks and Beyond

    … Extensive observations of unpolarized standard stars were carried out in the first six months of observing time at Ritter Observatory. The results of this effort has shown the polarimetric stability in the observations is at the same level or better compared to almost 10 years of observations at …

    ohiolink Repository record for A New Era of Observational Capability at Ritter Observatory: Spectropolarimetry from Exoplanets to Circumstellar Disks and Beyond (opens in a new tab)

  4. The formation and evolution of massive clusters in extragalactic environments

    … of clusters at young ages. The presence of Wolf-Rayet stars was also investigated within the clusters and the unreliability of Hα photometry in young cluster age and mass fitting was explored. Secondly, the cluster population of NGC 1566 was used to investigate the cluster mass function and …

    liverpool-jm Repository record for The formation and evolution of massive clusters in extragalactic environments (opens in a new tab)

  5. Hydrogen-deficient central stars of planetary nebulae

    Central stars of planetary nebulae are low-mass stars on the brink of their final evolution towards white dwarfs. Because of their surface temperature of above 25,000 K their UV radiation ionizes the surrounding material, which was ejected in an earlier phase of their evolution. Such fluorescent …

    potsdam-diss Repository record for Hydrogen-deficient central stars of planetary nebulae (opens in a new tab)