Table 3.
Novel or previously uncharacterized WDs recovered as OC members in the clustering analysis.
Gaia DR3 source_id | Associated OC | Pmax | Avail. photometry | MWD | tcool | Mi |
---|---|---|---|---|---|---|
(M⊙) | (Myr) | (M⊙) | ||||
2879428195013510144 | Alessi 22 | 1.0 | Gaia, PS, GALEX |
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4519349757798439936 | Alessi 62 | 0.8 | Gaia, PS, SDSS, GALEX |
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391939027303287040 | Alessi 94 | 1.0 | Gaia, PS |
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386116254240723712 | Alessi 94 | 1.0 | Gaia, PS |
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5798954758752816512 | CWNU 41 | 1.0 | Gaia |
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335525529520188032 | HSC 1155 | 1.0 | Gaia, PS |
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5257090272981848192 | HSC 2304 | 0.9 | Gaia |
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4502736137087916032 | HSC 381 | 0.9 | Gaia, PS, GALEX |
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6653882460188145152 | Mamajek 4 | 0.7 | Gaia, GALEX |
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4662157454731788672 | NGC 1901 | 0.6 | Gaia |
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4659513404187412736 | NGC 1901 | 0.8 | Gaia |
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2931807898171448320 | NGC 2358 | 0.8 | Gaia, PS |
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5289447182180342016 (a) | NGC 2516 | 0.9 | Gaia, GALEX |
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5294015515555860608 (a) | NGC 2516 | 1.0 | Gaia |
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5338675689360848256 | NGC 3532 | 0.6 | Gaia |
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5337742307052922752 | NGC 3532 | 0.8 | Gaia |
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5339898655484772864 | NGC 3532 | 0.8 | Gaia |
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5340530320614001792 | NGC 3532 | 0.5 | Gaia |
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5340165355769599744 | NGC 3532 | 0.6 | Gaia |
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4477168746525464064 (b) | NGC 6633 | 0.7 | Gaia, PS |
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4477214475044842368 (c) | NGC 6633 | 0.6 | Gaia, PS |
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342523646152426368 | NGC 752 | 0.7 | Gaia, PS, GALEX |
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4087833117945955840 | Ruprecht 147 | 0.7 | Gaia, PS, GALEX |
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4183928888026931328 | Ruprecht 147 | 0.9 | Gaia, PS |
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4183847562828165248 | Ruprecht 147 | 1.0 | Gaia, PS |
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4184148073089506304 | Ruprecht 147 | 0.8 | Gaia, PS |
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4183926006112672768 (d) | Ruprecht 147 | 0.9 | Gaia, PS |
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4184196073644880000 | Ruprecht 147 | 0.8 | Gaia, PS |
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507105143670906624 | Stock 2 | 0.5 | Gaia, PS |
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507555904779576064 | Stock 2 | 0.9 | Gaia, PS |
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506848643933335296 | Stock 2 | 0.6 | Gaia, PS |
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2174431990805230208 | Theia 248 | 1.0 | Gaia, PS |
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3324040907394753792 | Theia 558 | 1.0 | Gaia, PS, SDSS |
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4529222337115434240 | Theia 817 | 1.0 | Gaia, PS, SDSS |
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5433483136700686336 | Turner 5 | 0.7 | Gaia, GALEX |
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4098106821451715584 | UPK 5 | 0.8 | Gaia, PS |
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Notes. WD masses (MWD), cooling ages (tcool), and progenitor masses (Mi) have been calculated in Sect. 4. Pmax represents the maximum value of astrometric membership probability from P3D, P5D, and PHR.
Mentioned in Richer et al. (2021) but no Mi calculated,
possible double degenerate system (Williams et al. 2015),
radial velocity possibly inconsistent with OC membership (Williams et al. 2015),
approximate parameters derived also in Prišegen et al. (2021) using the GDR2 data.
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