Cite
VERIFYING ASTEROSEISMICALLY DETERMINED PARAMETERS OF KEPLER STARS USING HIPPARCOS PARALLAXES: SELF-CONSISTENT STELLAR PROPERTIES AND DISTANCES.
MLA
Silva Aguirre, V., et al. “Verifying Asteroseismically Determined Parameters of Kepler Stars Using Hipparcos Parallaxes: Self-Consistent Stellar Properties and Distances.” Astrophysical Journal, vol. 757, no. 1, Sept. 2012, p. 1. EBSCOhost, https://doi.org/10.1088/0004-637X/757/1/99.
APA
Silva Aguirre, V., Casagrande, L., Basu, S., Campante, T. L., Chaplin, W. J., Huber, D., Miglio, A., Serenelli, A. M., Ballot, J., Bedding, T. R., Christensen-Dalsgaard, J., Creevey, O. L., Elsworth, Y., García, R. A., Gilliland, R. L., Hekker, S., Kjeldsen, H., Mathur, S., Metcalfe, T. S., & Monteiro, M. J. P. F. G. (2012). Verifying Asteroseismically Determined Parameters of Kepler Stars Using Hipparcos Parallaxes: Self-Consistent Stellar Properties and Distances. Astrophysical Journal, 757(1), 1. https://doi.org/10.1088/0004-637X/757/1/99
Chicago
Silva Aguirre, V., L. Casagrande, S. Basu, T. L. Campante, W. J. Chaplin, D. Huber, A. Miglio, et al. 2012. “Verifying Asteroseismically Determined Parameters of Kepler Stars Using Hipparcos Parallaxes: Self-Consistent Stellar Properties and Distances.” Astrophysical Journal 757 (1): 1. doi:10.1088/0004-637X/757/1/99.