Image Details
Caption: Figure 5.
Gaia DR3 H-R diagram of CVs for which the orbital periods P orb are known in the final sample. The separating point of the orbital period gap is accepted as 2.6 hr (Ak et al. 2010). White dwarf and the main-sequence and giant star regions are shaded in blue and gray, respectively (Abril et al. 2020).
© 2023. The Author(s). Published by the American Astronomical Society.