BY Draconis variable (English Wikipedia)

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Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S. (2006), "Limits to Transits of the Neptune-mass planet orbiting Gl 581", Publications of the Astronomical Society of the Pacific, 118 (849): 1506, arXiv:astro-ph/0609255, Bibcode:2006PASP..118.1506L, doi:10.1086/508904, S2CID 15156619, BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.

Schrijver, Carolus J.; Zwaan, Cornelis (2000), Solar and stellar magnetic activity, Cambridge astrophysics series, vol. 34, Cambridge University Press, p. 343, ISBN 0-521-58286-5
Jaschek, Carlos; Jaschek, Mercedes (1990), The Classification of Stars, Cambridge University Press, p. 374, ISBN 0-521-38996-8

Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S. (2006), "Limits to Transits of the Neptune-mass planet orbiting Gl 581", Publications of the Astronomical Society of the Pacific, 118 (849): 1506, arXiv:astro-ph/0609255, Bibcode:2006PASP..118.1506L, doi:10.1086/508904, S2CID 15156619, BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.

Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S. (2006), "Limits to Transits of the Neptune-mass planet orbiting Gl 581", Publications of the Astronomical Society of the Pacific, 118 (849): 1506, arXiv:astro-ph/0609255, Bibcode:2006PASP..118.1506L, doi:10.1086/508904, S2CID 15156619, BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.

Lopez-Morales, Mercedes; Morrell, N. I.; Butler, R. P.; Seager, S. (2006), "Limits to Transits of the Neptune-mass planet orbiting Gl 581", Publications of the Astronomical Society of the Pacific, 118 (849): 1506, arXiv:astro-ph/0609255, Bibcode:2006PASP..118.1506L, doi:10.1086/508904, S2CID 15156619, BY Draconis variable. This type of variable is characterized by quasiperiodic photometric variations over time scales from less than a day to months, and amplitudes ranging from a few hundredths of a magnitude to 0.5 mags.