Very regular high-frequency pulsation modes in young intermediate-mass stars (IMAGE)
Caption
Still image from animation showing a simulation of pulsations in the delta Scuti variable star called HD 31901, based on brightness measurements by NASA's Transiting Exoplanet Survey Satellite (TESS).
Credit
Credit: produced by Dr Chris Boshuizen (twitter.com/DrChrispyMusic or instagram.com/DrChrispyMusic), with assistance from Dr Simon Murphy and Prof. Tim Bedding (twitter.com/timbedding).
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