Pulsating low-mass white dwarfs in the frame of new evolutionary sequences - V. Asteroseismology of ELMV white dwarf stars

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Table 29

Stellar masses (in solar units) for all of the studied ELMV WD stars.


Star		Period fit		Spectroscopy


	ℓ = 1	ℓ = 1,2	ℓ = 1,2(g,p)	(other works)
	(g)	(g)	ℓ = 0 (radial)	1D	3D


J1840	0.2389	0.1805	–	0.183^a	0.177^f
J1112	0.3205^*	0.2389^*	0.1612^**	0.179^b	0.169^f
J1518	0.3205	0.2707	–	0.220^b	0.197^f
J1614	0.1762	0.3205	–	0.192^c	0.172^f
J2228	0.1650	0.1554	–	0.152^c	0.142^f
J1738	0.4352	0.4352	–	0.181^d	0.172^f
J1618	0.2019	0.1706	–	0.220^e	0.179^f
J1735	0.3624	0.1612	–	–	0.142^g
J2139	0.1863	–	–	–	0.149^g

Notes.

^(*)

Determined using a subset of the observed periods.

^(**)

Determined using the whole set of the observed periods.

^(a)

Hermes et al. (2012).

^(b)

Hermes et al. (2013b).

^(c)

Hermes et al. (2013a).

^(d)

Kilic et al. (2015).

^(e)

Bell et al. (2015).

^(f)

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

^(g)

Bell et al. (2017).

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