Pulsating low-mass white dwarfs in the frame of new evolutionary sequences - VI. Thin H-envelope sequences and asteroseismology of ELMV stars revisited

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Table 2.

Stellar parameters derived using 1D and 3D model atmospheres of the ELMVs shown in this work.

Star		log(g)^1D			log(g)^3D
	(K)	(cgs)	(M_⊙)	(K)	(cgs)	(M_⊙)
J1112	9590 ± 140	6.36 ± 0.06	0.179^a	9240 ± 140	6.17 ± 0.06	0.169^b
J1518	9900 ± 140	6.80 ± 0.05	0.220^a	9650 ± 140	6.68 ± 0.05	0.197^b
J1738	9130 ± 140	6.55 ± 0.06	0.181^c	8910 ± 150	6.30 ± 0.10	0.172^b
J1735	–	–	–	7940 ± 130	5.76 ± 0.08	0.142^d

Notes.

^(a)

Hermes et al. (2013b).

^(b)

Determined using the corrections for 3D effects by Tremblay et al. (2015).

^(c)

Kilic et al. (2015).

^(d)

Bell et al. (2017).

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