Light curves and Fourier amplitude spectra for the three new pulsating low-mass white dwarfs

Light curves (left) and Fourier amplitude spectra (right) for the three new pulsating low-mass white dwarfs. The red tick marks denote the significant frequencies which lie above the detection threshold of four times the average noise level.

Credit:

International Gemini Observatory/NOIRLab/NSF/AURA

About the Image

Id:geminiann16008a
Type:Chart
Release date:May 11, 2016, 1:02 p.m.
Related announcements:geminiann16008
Size:500 x 374 px

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