APA (7th ed.) Citation

Takahashi, K., & Langer, N. (2024). Standing torsional Alfvén waves as the source of the rotational period variation in magnetic early-type stars.

Chicago Style (17th ed.) Citation

Takahashi, Koh, and Norbert Langer. Standing Torsional Alfvén Waves as the Source of the Rotational Period Variation in Magnetic Early-type Stars. 2024.

MLA (9th ed.) Citation

Takahashi, Koh, and Norbert Langer. Standing Torsional Alfvén Waves as the Source of the Rotational Period Variation in Magnetic Early-type Stars. 2024.

Warning: These citations may not always be 100% accurate.