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An approximation to determine the source of the WOW! Signal
Alberto Caballero, 2022. International Journal of Astrobiology.
Samples 66 G and K stars in the Wow! region from the Gaia archive and names one, 2MASS 19281982−2640123, as the best Sun-like candidate if the signal came from a star system like ours. IJA 21, 129–136.
What it's used for here
The only published attempt to name a stellar candidate; depends on assumptions the paper states.
Our copy
Research copy, for editors and curators. The work is the publisher's, so readers are sent to it. We keep this copy so the citation can be checked if the page changes or goes.
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The Wow! signal
MYSThe mystery article
Cite it
Caballero, A. (2022). An approximation to determine the source of the WOW! Signal. International Journal of Astrobiology. https://doi.org/10.1017/S1473550422000015
@article{caballero2022approximation,
author = {Caballero, Alberto},
title = {An approximation to determine the source of the WOW! Signal},
journal = {International Journal of Astrobiology},
year = {2022},
doi = {10.1017/S1473550422000015},
url = {https://doi.org/10.1017/S1473550422000015}
}TY - JOUR TI - An approximation to determine the source of the WOW! Signal AU - Caballero, Alberto PY - 2022 JO - International Journal of Astrobiology DO - 10.1017/S1473550422000015 UR - https://doi.org/10.1017/S1473550422000015 ER -
Caballero, Alberto. “An approximation to determine the source of the WOW! Signal.” International Journal of Astrobiology (2022). https://doi.org/10.1017/S1473550422000015.