Publication Abstracts
Hudson et al. 1971
Hudson, K.I., H.-Y. Chiu, S.P. Maran, F.E. Stuart, and P.R. Vokac, 1971: Automated and conventional photometry of the short-period variable star 14 Aurigae. Astrophys. J., 165, 573-580, doi:10.1086/150922.
Amplitude of the V-light curve of the δ Scuti star 14 Aurigae varied from 0.02 to 0.08 mag on six nights. The changes in amplitude accompanied comparable changes in maximum brightness, wheras changes in minimum brightness were much smaller. The light period is 0.08748 d, and the spectroscopic-binary period is 3.788506 d. Small variations in color indices, associated with the light variation, resemble those of other δ Scuti stars. The use of an automated telescope was effective in obtaining large number of routine observations.
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BibTeX Citation
@article{hu06000k,
author={Hudson, K. I. and Chiu, H.-Y. and Maran, S. P. and Stuart, F. E. and Vokac, P. R.},
title={Automated and conventional photometry of the short-period variable star 14 Aurigae},
year={1971},
journal={Astrophysical Journal},
volume={165},
pages={573--580},
doi={10.1086/150922},
}
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RIS Citation
TY - JOUR ID - hu06000k AU - Hudson, K. I. AU - Chiu, H.-Y. AU - Maran, S. P. AU - Stuart, F. E. AU - Vokac, P. R. PY - 1971 TI - Automated and conventional photometry of the short-period variable star 14 Aurigae JA - Astrophys. J. JO - Astrophysical Journal VL - 165 SP - 573 EP - 580 DO - 10.1086/150922 ER -
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