Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Kuszlewicz, J. S."'
Publikováno v:
A&A 640, A130 (2020)
Stars of low and intermediate mass that exhibit oscillations may show tens of detectable oscillation modes each. Oscillation modes are a powerful to constrain the internal structure and rotational dynamics of the star, hence tool allowing one to obta
Externí odkaz:
http://arxiv.org/abs/2006.08245
Autor:
Rendle, B. M., Buldgen, G., Miglio, A., Reese, D., Noels, A., Davies, G. R., Campante, T. L., Chaplin, W. J., Lund, M. N., Kuszlewicz, J. S., Scott, L. J. A., Scuflaire, R., Ball, W. H., Smetana, J., Nsamba, B.
A key aspect in the determination of stellar properties is the comparison of observational constraints with predictions from stellar models. Asteroseismic Inference on a Massive Scale (AIMS) is an open source code that uses Bayesian statistics and a
Externí odkaz:
http://arxiv.org/abs/1901.02663
Stars are stretched by tidal interactions in tight binaries, and changes to their projected areas introduce photometric variations twice per orbit. Hermes et al. (2014, ApJ, 792, 39) utilized measurements of these ellipsoidal variations to constrain
Externí odkaz:
http://arxiv.org/abs/1809.05623
Autor:
Campante, T. L., Schofield, M., Kuszlewicz, J. S., Bouma, L., Chaplin, W. J., Huber, D., Christensen-Dalsgaard, J., Kjeldsen, H., Bossini, D., North, T. S. H., Appourchaux, T., Latham, D. W., Pepper, J., Ricker, G. R., Stassun, K. G., Vanderspek, R., Winn, J. N.
New insights on stellar evolution and stellar interiors physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also played an important role in the characterization of exoplanet-host sta
Externí odkaz:
http://arxiv.org/abs/1608.01138
Autor:
Miglio, A., Chaplin, W. J., Brogaard, K., Lund, M. N., Mosser, B., Davies, G. R., Handberg, R., Milone, A. P., Marino, A. F., Bossini, D., Elsworth, Y. P., Grundahl, F., Arentoft, T., Bedin, L. R., Campante, T. L., Jessen-Hansen, J., Jones, C. D., Kuszlewicz, J. S., Malavolta, L., Nascimbeni, V., Sandquist, E. L.
Asteroseismic constraints on K giants make it possible to infer radii, masses and ages of tens of thousands of field stars. Tests against independent estimates of these properties are however scarce, especially in the metal-poor regime. Here, we repo
Externí odkaz:
http://arxiv.org/abs/1606.02115
Autor:
Campante, T. L., Lund, M. N., Kuszlewicz, J. S., Davies, G. R., Chaplin, W. J., Albrecht, S., Winn, J. N., Bedding, T. R., Benomar, O., Bossini, D., Handberg, R., Santos, A. R. G., Van Eylen, V., Basu, S., Christensen-Dalsgaard, J., Elsworth, Y. P., Hekker, S., Hirano, T., Huber, D., Karoff, C., Kjeldsen, H., Lundkvist, M. S., North, T. S. H., Aguirre, V. Silva, Stello, D., White, T. R.
The angle $\psi$ between a planet's orbital axis and the spin axis of its parent star is an important diagnostic of planet formation, migration, and tidal evolution. We seek empirical constraints on $\psi$ by measuring the stellar inclination $i_{\rm
Externí odkaz:
http://arxiv.org/abs/1601.06052
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