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Map of the most intrinsically luminous stars within 100 parsecs from the Gaia Catalogue of Nearby Stars (based on Gaia EDR3). Also includes the Spica and zeta Ophiuchi nebulae, and several star density structures including the Hyades, the Coma Berenices star cluster, the Ursa Major moving group, the Tucana-Horologium association, the eta Chamaeleontis association and the 32 Orionis group. The map background shows OB star density isosurfaces from Gaia DR3.
{"references": ["Smart, Richard Laurence, et al. \"Gaia Early Data Release 3-The Gaia Catalogue of Nearby Stars.\" Astronomy & Astrophysics 649 (2021): A6.", "Drimmel, Ronald, et. al. \"Gaia Data Release 3: Mapping the asymmetric disc of the Milky Way\", arXiv:2206.06207"]}
Cartography, Gaia EDR3, Gaia DR3
Cartography, Gaia EDR3, Gaia DR3
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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| downloads | 38 |

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