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Showing 1 to 8 of 8 for “"Late-type stars"”.

  1. Zeeman-Doppler Imaging of active late-type stars

    Stellare Magnetfelder spielen eine wichtige Rolle bei der Entstehung und Entwicklung von Sternen. Leider entziehen sie sich aber, aufgrund ihrer großen Entfernung zur Erde, einer direkten Beobachtung. Dies gilt zumindest für derzeitige und in naher Zukunft zur Verfügung stehende Instrumente. Um …

    potsdam-diss Repository record for Zeeman-Doppler Imaging of active late-type stars (opens in a new tab)

  2. The chemistry of metal-containing molecules in the circumstellar envelopes of late-type stars: Millimeter-wave observations and abundance modeling

    … of Asymptotic Giant Branch (AGB) and post-AGB stars has been conducted in order to investigate the role of metal-containing compounds in the circumstellar envelopes surrounding these objects. The role of metal bearing molecules in the chemical evolution of these envelopes was also examined. …

    arizona-thes Repository record for The chemistry of metal-containing molecules in the circumstellar envelopes of late-type stars: Millimeter-wave observations and abundance modeling (opens in a new tab)

  3. Generation and propagation of longitudinal tube waves in late-type stellar atmospheres and the rotation-emission activity relation

    … the turbulent medium of the convection zones of late-type stars were computed. Solar magnetic flux tubes of different filling factors were heated with adiabatic and radiatively damped LTW. It was found that the tube geometry plays an important role for heating the outer layers. The response of …

    heid-diss Repository record for Generation and propagation of longitudinal tube waves in late-type stellar atmospheres and the rotation-emission activity relation (opens in a new tab)

  4. Planets around cool stars: a spectroscopic and photometric study of M dwarfs and their planets

    … searches. Smaller planets can be detected around stars with smaller radii (via the transit technique) or lower mass (via the radial velocity technique). Planets in the habitable zone of an M dwarf are closer in, and thus easier to detect, than those orbiting in the habitable zone of Solar-type

    hawaii Repository record for Planets around cool stars: a spectroscopic and photometric study of M dwarfs and their planets (opens in a new tab)

  5. Massive stars in the Galactic Center Quintuplet 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 region …

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

  6. The Structure and Polarization Properties of the SiO Masers in the Extended Atmosphere of R Aquarii

    … maser emission has been observed towards many late-type stars. The conditions necessary for the formation of SiO masers dictate that they be produced in a region which is inside the silicate dust formation point close to the surface of the star. Very Long Baseline Interferometry (VLBI) has …

    vt Repository record for The Structure and Polarization Properties of the SiO Masers in the Extended Atmosphere of R Aquarii (opens in a new tab)

  7. Chromospheric activity and lithium abundance in the NGC2516 and NGC3766 open clusters

    … chromospheric activity and lithium abundance of late type stars in open clusters of different ages. The study of open cluster is very important for our understanding of stellar evolution and atmospheres, since all cluster members have almost the same age and chemical composition and this allows …

    catania Repository record for Chromospheric activity and lithium abundance in the NGC2516 and NGC3766 open clusters (opens in a new tab)