STARS, GAS, AND DARK MATTER IN THE SOLAR NEIGHBORHOOD
Open accessAbstract
We reanalyze data on the surface densities and vertical distribution of baryonic matter in the solar neighborhood and tabulate the results. We find a local total surface density of M dwarfs of , whcih is significantly higher than previous values. Our result for the total local surface density of visible stars (main-sequence stars and giants), , is close to previous estimates due to a cancellation of opposing effects: more mass in M dwarfs, less mass in the others. The total local surface density in white dwarfs is ; in brown dwarfs, it is , but with considerable uncertainty. We find that the total local surface density of stars and stellar remnants is , which is somewhat less than previous estimates but within the errors of many of them. We analyze data on 21 cm emission and absorption and obtain good agreement with recent results on the local amount of neutral atomic hydrogen obtained with the Planck satellite. The local surface density of gas is . The total baryonic mass surface density that we derive for the solar neighborhood is ( within 1.1 kpc of the midplane). Combining these results with others' measurements of the total surface density of matter within 1–1.1 kpc of the plane, we find that the local density of dark matter is GeV cm . The local density of all matter is . We discuss limitations on the properties of a possible thin disk of dark matter.
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The two recent determinations of Read (2014) and McKee et al. (2015) favour the contracted halo model; however, due to large uncertainties, the pure NFW model cannot be ruled out.
“The two recent determinations of Read (2014) and McKee et al. (2015) favour the contracted halo model; however, due to large uncertainties, the pure NFW model cannot be ruled out.”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as McKee et al. (2015)
Split into 2 atoms — 0 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 1 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredThe local total surface mass density Σ is given by McKee et al. (2015).
“which is given by (McKee et al. 2015)”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as McKee et al. 2015
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The Galaxy in Context: Structural, Kinematic, and Integrated Properties
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“(53) from McKee et al. (2015), combined with the Eilers et al. (2019) rotation curve to obtain ∆Σ = 9 M pc−2.”
BackgroundMethodOn the estimation of the local dark matter density using the rotation curve of the Milky Way
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INTERACTION CROSS SECTIONS AND SURVIVAL RATES FOR PROPOSED SOLAR SYSTEM MEMBER PLANET NINE
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Geometry-driven and dark-matter-sustained Milky Way rotation curves with <i>Gaia</i> DR3
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MICROSCOPE’s view at gravitation
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- Authors
- McKee, C. F., Parravano, A., & Hollenbach, D. J.
- Affiliations
- University of California, Berkeley (US)
- Universidad de Los Andes (VE)
- Search for Extraterrestrial Intelligence (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2015-11-12
- Volume
- 814
- Issue
- 1
- Pages
- 13
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1864516950
- Cited by
- 270
- References
- 129
- Citations by year
- 2026: 10 · 2025: 32 · 2024: 24 · 2023: 19 · 2022: 31 · 2021: 44 · 2020: 31 · 2019: 14 · 2018: 23 · 2017: 16 · 2016: 26
- FWCI
- 12.33
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- solar neighborhood, baryonic surface density, dark matter density, M dwarfs, white dwarfs, brown dwarfs, stellar remnants, neutral hydrogen, HI 21 cm emission, Planck, local matter density
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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