Cite
HARVARD Citation
Samec, R. et al. (2019). V1187 Herculis: A Red Novae progenitor, and the most extreme mass ratio binary known. Proceedings of the International Astronomical Union. pp. 288-293. [Online].
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Samec, R. et al. (2019). V1187 Herculis: A Red Novae progenitor, and the most extreme mass ratio binary known. Proceedings of the International Astronomical Union. pp. 288-293. [Online].