Table 3.

List of known MWDs younger than 0.5 Gyr within 40 pc from the Sun.

〈|B|〉M
Star(MG)(M)ReferencesNotes
WD 0041−102201.1Liebert et al. (1977)
WD 0232+5250.005:0.82Unpublished
WD 0301+0592001.12Landstreet & Bagnulo (2020)
WD 0316−8493000.86Barstow et al. (1995)1
WD 0945+2456700.80Liebert et al. (1993)
WD 1105−0480.010:0.58Aznar Cuadrado et al. (2004)
WD 1105−3400.1500.67Landstreet & Bagnulo (2019a)
WD 1658+4402.31.32Schmidt et al. (1992)
WD 2047+3720.060.82Landstreet et al. (2017)
〈|B|〉M
Star(MG)(M)ReferencesNotes
WD 0041−102201.1Liebert et al. (1977)
WD 0232+5250.005:0.82Unpublished
WD 0301+0592001.12Landstreet & Bagnulo (2020)
WD 0316−8493000.86Barstow et al. (1995)1
WD 0945+2456700.80Liebert et al. (1993)
WD 1105−0480.010:0.58Aznar Cuadrado et al. (2004)
WD 1105−3400.1500.67Landstreet & Bagnulo (2019a)
WD 1658+4402.31.32Schmidt et al. (1992)
WD 2047+3720.060.82Landstreet et al. (2017)

Note. 1. Star WD 0316−849 = RE J0317−853 = EUVE J0317−853 = V* CL Oct is often confused with star WD 0325−857 = EQ J0317−855 = LB 9802, a hot and young non-MWD (Kawka et al. 2007, table 1).

Table 3.

List of known MWDs younger than 0.5 Gyr within 40 pc from the Sun.

〈|B|〉M
Star(MG)(M)ReferencesNotes
WD 0041−102201.1Liebert et al. (1977)
WD 0232+5250.005:0.82Unpublished
WD 0301+0592001.12Landstreet & Bagnulo (2020)
WD 0316−8493000.86Barstow et al. (1995)1
WD 0945+2456700.80Liebert et al. (1993)
WD 1105−0480.010:0.58Aznar Cuadrado et al. (2004)
WD 1105−3400.1500.67Landstreet & Bagnulo (2019a)
WD 1658+4402.31.32Schmidt et al. (1992)
WD 2047+3720.060.82Landstreet et al. (2017)
〈|B|〉M
Star(MG)(M)ReferencesNotes
WD 0041−102201.1Liebert et al. (1977)
WD 0232+5250.005:0.82Unpublished
WD 0301+0592001.12Landstreet & Bagnulo (2020)
WD 0316−8493000.86Barstow et al. (1995)1
WD 0945+2456700.80Liebert et al. (1993)
WD 1105−0480.010:0.58Aznar Cuadrado et al. (2004)
WD 1105−3400.1500.67Landstreet & Bagnulo (2019a)
WD 1658+4402.31.32Schmidt et al. (1992)
WD 2047+3720.060.82Landstreet et al. (2017)

Note. 1. Star WD 0316−849 = RE J0317−853 = EUVE J0317−853 = V* CL Oct is often confused with star WD 0325−857 = EQ J0317−855 = LB 9802, a hot and young non-MWD (Kawka et al. 2007, table 1).

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