Photometric Variability of the Be Star Population. Labadie-Bartz, J., Pepper, J., McSwain, M. V., Bjorkman, J., Bjorkman, K., Lund, M. B., Rodriguez, J. E., Stassun, K. G., Stevens, D. J., James, D. J., Kuhn, R. B., Siverd, R. J., & Beatty, T. G. \aj, 153(6):252, June, 2017. doi bibtex @ARTICLE{2017AJ....153..252L,
author = {{Labadie-Bartz}, Jonathan and {Pepper}, Joshua and {McSwain}, M. Virginia and {Bjorkman}, J.~E. and {Bjorkman}, K.~S. and {Lund}, Michael B. and {Rodriguez}, Joseph E. and {Stassun}, Keivan G. and {Stevens}, Daniel J. and {James}, David J. and {Kuhn}, Rudolf B. and {Siverd}, Robert J. and {Beatty}, Thomas G.},
title = "{Photometric Variability of the Be Star Population}",
journal = {\aj},
keywords = {stars: emission-line, Be, stars: oscillations, stars: variables: general, techniques: photometric, techniques: spectroscopic, Astrophysics - Solar and Stellar Astrophysics},
year = 2017,
month = jun,
volume = {153},
number = {6},
eid = {252},
pages = {252},
doi = {10.3847/1538-3881/aa6396},
archivePrefix = {arXiv},
eprint = {1609.08449},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2017AJ....153..252L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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