Ages τ★ (in Myr), masses M★ (in solar masses) and spectral types (SpT) for 7663 young stars (sorted by their HIP number). τ★ and M★ are medians obtained from different evolutionary models (see Section 2.1). For 2250 stars, only the spectral type is given as models infer a larger age; however, these are probably also young (as inferred from the spectral type and luminosity class). The first five entries are shown here; the full table is available as Supporting Information with the article, and via VizieR.
HIP | Other name | τ★ (Myr) | M★ (M⊙) | SpT |
32 | HD 224756 | 10.0 ± 7.6 | 2.8 ± 0.1 | B8 |
85 | CD-25 16747 | 39.8 ± 28.8 | 1.8 ± 0.1 | A2 |
106 | HD 224870 | – | – | G7II–III |
124 | HD 224893 | 44.7 ± 5.4 | 7.6 ± 0.4 | F0III |
135 | HD 224908 | 45.7 ± 22.9 | 1.0 ± 0.1 | G5 |
HIP | Other name | τ★ (Myr) | M★ (M⊙) | SpT |
32 | HD 224756 | 10.0 ± 7.6 | 2.8 ± 0.1 | B8 |
85 | CD-25 16747 | 39.8 ± 28.8 | 1.8 ± 0.1 | A2 |
106 | HD 224870 | – | – | G7II–III |
124 | HD 224893 | 44.7 ± 5.4 | 7.6 ± 0.4 | F0III |
135 | HD 224908 | 45.7 ± 22.9 | 1.0 ± 0.1 | G5 |
Ages τ★ (in Myr), masses M★ (in solar masses) and spectral types (SpT) for 7663 young stars (sorted by their HIP number). τ★ and M★ are medians obtained from different evolutionary models (see Section 2.1). For 2250 stars, only the spectral type is given as models infer a larger age; however, these are probably also young (as inferred from the spectral type and luminosity class). The first five entries are shown here; the full table is available as Supporting Information with the article, and via VizieR.
HIP | Other name | τ★ (Myr) | M★ (M⊙) | SpT |
32 | HD 224756 | 10.0 ± 7.6 | 2.8 ± 0.1 | B8 |
85 | CD-25 16747 | 39.8 ± 28.8 | 1.8 ± 0.1 | A2 |
106 | HD 224870 | – | – | G7II–III |
124 | HD 224893 | 44.7 ± 5.4 | 7.6 ± 0.4 | F0III |
135 | HD 224908 | 45.7 ± 22.9 | 1.0 ± 0.1 | G5 |
HIP | Other name | τ★ (Myr) | M★ (M⊙) | SpT |
32 | HD 224756 | 10.0 ± 7.6 | 2.8 ± 0.1 | B8 |
85 | CD-25 16747 | 39.8 ± 28.8 | 1.8 ± 0.1 | A2 |
106 | HD 224870 | – | – | G7II–III |
124 | HD 224893 | 44.7 ± 5.4 | 7.6 ± 0.4 | F0III |
135 | HD 224908 | 45.7 ± 22.9 | 1.0 ± 0.1 | G5 |
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