Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis
- DOI
- 10.1086/313123
- Published
- 1998-08
- Container
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Open access
- unknown
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Cite this work
BibTeX
@article{allodium:10.1086/313123,
title = {Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis},
author = {Timothy M. Brown and Rubina Kotak and Scott D. Horner and Edward J. Kennelly and Sylvain Korzennik and P. Nisenson and Robert W. Noyes},
year = {1998},
journal = {The Astrophysical Journal Supplement Series},
doi = {10.1086/313123},
url = {https://doi.org/10.1086/313123}
}RIS
TY - JOUR TI - Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis AU - Timothy M. Brown AU - Rubina Kotak AU - Scott D. Horner AU - Edward J. Kennelly AU - Sylvain Korzennik AU - P. Nisenson AU - Robert W. Noyes PY - 1998 JO - The Astrophysical Journal Supplement Series DO - 10.1086/313123 UR - https://doi.org/10.1086/313123 ER -
APA
Brown, T. M., Kotak, R., Horner, S. D., Kennelly, E. J., Korzennik, S., Nisenson, P., & Noyes, R. W. (1998). Exoplanets or Dynamic Atmospheres? The Radial Velocity and Line Shape Variations of 51 Pegasi and τ Bootis. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/313123
Source records
- crossref · retrieved 2026-09-25T16:18:44.293Z