Blue large-amplitude pulsators formed from the merger of low-mass white dwarfs

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Table 1.

Fundamental properties of the three models of merging DELM WDs analysed in our study.

Model	M_ini (M_⊙) ^(*)	M_HeWD, 1 + M_HeWD, 2 (M_⊙) ^(**)
A	1.2	0.16 + 0.16 (0.32)
B	1.5	0.20 + 0.20 (0.40)
C	2.5	0.35 + 0.35 (0.70)

Notes.

^(*)

Initial mass of the MS star that evolved to RGB to obtain the model of ELM WD.

^(**)

Masses of the two DELM WD components whose mergers are analysed in this study. The mass of the resulting BLAP is given in parentheses.

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