Spectral evolution of hot hybrid white dwarfs - I. Spectral analysis

Open Access

Table B.3

Previous analyses whose results are compared to the DAO WDs in our sample.

Name	Optical	UV	Optical + UV	Abundances
DAO
Longmore 1	⁽¹⁾	^{(2), (3)}	−	^{(2), (3)}
WD 0439+466	^{(4), (5), (6)}	⁽⁷⁾	⁽⁸⁾	^{(7), (8)}
WD 0500–156	^{(5), (6), (9), (10), (11), (12)}	^{(3), (12)}	−	^{(3), (13)}
WD 0615+556	^{(5), (6), (11), (12)}	^{(3), (12)}	−	^{(3), (13)}
WD 0823+316	^{(4), (6), (12), (14), (15), (16)}	⁽¹²⁾	−	⁽¹³⁾
WD 0834+500	^{(4), (6), (12)}	⁽¹²⁾	−	⁽¹³⁾
WD 0851+090	^{(5), (12)}	^{(3), (12)}	−	^{(3), (13)}
WD 1111+552	^{(5), (11)}	⁽³⁾	−	⁽³⁾
WD 1214+267	^{(4), (6), (12), (17)}	⁽¹²⁾	−	⁽¹³⁾
WD 1253+378	^{(4), (5), (6), (10), (12), (18)}	⁽¹²⁾	−	⁽¹³⁾
WD 1957+225	^{(5), (6)}	⁽⁷⁾	⁽³⁾	^{(3), (7)}
WD 2226–210	^{(1), (5), (6), (11), (19)}	⁽⁷⁾	⁽³⁾	^{(3), (7)}
WD 2342+806	^{(4), (5), (6), (12)}	^{(3), (12)}	−	^{(3), (13)}

References. ⁽¹⁾ Mendez et al. (1985), ⁽²⁾ Herald & Bianchi (2004), ⁽³⁾ Ziegler (2012), ⁽⁴⁾ Bergeron et al. (1994), ⁽⁵⁾ Napiwotzki (1999), ⁽⁶⁾ Gianninas et al. (2010), ⁽⁷⁾ Traulsen et al. (2005), ⁽⁸⁾ Rauch et al. (2007), ⁽⁹⁾ Mendez et al. (1981), ⁽¹⁰⁾ Wesemael et al. (1985), ⁽¹¹⁾ McCarthy et al. (1997), ⁽¹²⁾ Good et al. (2004), ⁽¹³⁾ Good et al. (2005b), ⁽¹⁴⁾ Tremblay et al. (2011), ⁽¹⁵⁾ Kepler et al. (2019), ⁽¹⁶⁾ Bédard et al. (2020), ⁽¹⁷⁾ Guo et al. (2015), ⁽¹⁸⁾ Lei et al. (2023), ⁽¹⁹⁾ Mendez et al. (1988).

Notes. The second and third columns list studies that only utilized optical and UV data, respectively, or the analyses derived separate parameters for both wavebands, whereas the fourth column displays the ones that reached a common T_eff and log g from both wavelength ranges. The fifth column lists works that performed abundance analyses.

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