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Showing 1 to 10 of 10 for “"stellar rotation"”.

  1. An analysis of beta cephei stars in NGC 3293 and the effects of stellar rotation

    … predictions, including the effects of rotation. The results imply a preference for first and second overtone quadrupole (l=2) pulsation in these stars, while a weak relationship between stellar mass and pulsation overtone is identified. One of the stars is identified as a member of an …

    cape-town Repository record for An analysis of beta cephei stars in NGC 3293 and the effects of stellar rotation (opens in a new tab)

  2. Unearth: Revealing the Effects of Stellar Activity on Exoplanet Host Stars

    … thesis, I investigate the effect activity has on stellar spectra, using HARPS data of the well observed K1 V star α Centauri B. I compare spectra from high- and low-activity periods (as traced by log R′HK) of α Cen B. I produce ‘relative spectra’ by dividing the high-activity spectra by a …

    qu-belfast Repository record for Unearth: Revealing the Effects of Stellar Activity on Exoplanet Host Stars (opens in a new tab)

  3. Constraining Stellar Evolution in Young Open Clusters with NGTS

    Understanding stellar evolution is fundamental to astronomy, yet there remain significant gaps in our knowledge. Scientific progress requires testing our best explanations against observation, and open clusters act as key test sites for theories of stellar evolution. Observations of young open …

    cambridge Repository record for Constraining Stellar Evolution in Young Open Clusters with NGTS (opens in a new tab)

  4. Exoplanetary system WASP-3 : measurement of the projected spin-orbit angle and evidence for stellar activity

    … angle between the planetary orbital axis and the stellar rotation axis, ... degrees. I use the new photometric data to refine the system parameters. Additionally, I present evidence for stellar activity, as the spectra obtained on UT June 19, 2008 reveal an increase in radial velocity to a peak …

    mit Repository record for Exoplanetary system WASP-3 : measurement of the projected spin-orbit angle and evidence for stellar activity (opens in a new tab)

  5. K-Star rapid rotators and the detection of relatively young multiple K-Star systems

    … evidence of periodicities that indicate rapid stellar rotation. Many Kepler M, K, and G stars show modulations in flux due to rotating star spots, and these have been previously investigated by a number of different groups. Rotational periodicities mediated by the rotation of stellar spots were …

    mit Repository record for K-Star rapid rotators and the detection of relatively young multiple K-Star systems (opens in a new tab)

  6. Em busca de um novo indicador Espectroscópico do período de rotação das Estrelas do tipo solar

    … with the dynamics of sunspots that the Sun has a rotation period of twenty-seven days around your axis. With the help of Project Sun-As-A-Star that solar spectra obtained for more than thirty years we observed oscillations of both the depth of the spectral line and its equivalent width, and …

    brazil-ufrn Repository record for Em busca de um novo indicador Espectroscópico do período de rotação das Estrelas do tipo solar (opens in a new tab)

  7. Motion of charged particles in pulsar magnetospheres

    … view: (i) For the case of aligned magnetic and rotational axes we solve a fluid version of the Lorentz-Dirac equation, in the Landau approximation, for a two-component plasma. We start from an approximately force-free initial condition and numerically integrate the equations of motion for a time …

    uiuc Repository record for Motion of charged particles in pulsar magnetospheres (opens in a new tab)

  8. Multi-dimensional simulations of bow shocks of massive, high-velocity runaway stars

    Stellar bow shocks result from the supersonic collision of stellar winds ejected by runaway stars and the interstellar medium (ISM). Studying their properties provides constraints on mass-loss rates, stellar wind velocities and the properties of the ISM. In this work, we study the formation of bow …

    cape-town Repository record for Multi-dimensional simulations of bow shocks of massive, high-velocity runaway stars (opens in a new tab)

  9. Ground-based transmission spectroscopy of three inflated Hot Jupiter exoplanets

    … photometrically to correct for influences of stellar activity if necessary. The obtained measurements of the three objects all favor featureless spectra. A variety of atmospheric compositions can explain the lack of a wavelength dependent absorption. But the broad trend of featureless spectra …

    potsdam-diss Repository record for Ground-based transmission spectroscopy of three inflated Hot Jupiter exoplanets (opens in a new tab)

  10. Variability of young solar-type stars : Spot cycles, rotation, and active longitudes

    … fields. When these magnetic fields penetrate the stellar surface, they give rise to directly observable activity phenomena, such as dark spots and line emission from the chromospheric layers. Observing and analyzing these activity indicators allows us to characterize the behaviour of the dynamos …

    helsinki Repository record for Variability of young solar-type stars : Spot cycles, rotation, and active longitudes (opens in a new tab)