The galactic disk surface mass density and the Galactic force K(z) at Z = 1.1 kiloparsecs
Abstract
A set of distance and velocity data previously obtained and analyzed is rediscussed to determine the surface mass density of the Galactic disk. These data reliably determine the integral surface mass density of all (disk + halo) Galactic components within 1.1 kpc from the Galactic plane near the sun to be 71 + or 6 solar masses/sq pc, independent of the disk/halo ratio. Determination of the fraction of this total mass which is distributed in the Galactic disk and the fraction which is associated with an extended halo remains highly model-dependent. The best available estimate of the relative contributions of disk mass and halo mass to the local integral surface density, obtained from modeling of the Galactic rotation curve, yields a surface mass density of 48 + or - 9 solar masses/sq pc for mass associated with the Galactic disk near the sun. The corresponding mass of identified disk matter is 48 + or - 8 solar masses/sq pc.
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The vertical force at 1.1 kpc above the plane at the Sun's position is taken as (Kuijken & Gilmore 1991).
“The last measurement we consider is the value of the vertical force at 1 . 1 kpc above the plane at the Sun's position, which we take as (Kuijken & Gilmore 1991)”
From The milky way total mass profile as inferred from Gaia DR2 (2020) · cites this paper as Kuijken & Gilmore 1991
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Read, J. I. (2014) · Journal of Physics G: Nuclear and Particle Physics · doi:10.1088/0954-3899/41/6/063101 · Cited by 489 · see citing works
The milky way total mass profile as inferred from Gaia DR2
Cautun, M., Benítez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa1017 · Cited by 332 · see citing works
“The last measurement we consider is the value of the vertical force at 1.1 kpc above the plane at the Sun’s position, which we take as (Kuijken & Gilmore 1991) : Kz(R ) = 2πG× (71± 6) M pc−2 .”
MethodInfluentialThe Milky Way total mass profile as inferred from Gaia DR2
Cautun, M., Benitez-Llambay, A., Deason, A. J., Frenk, C. S., Fattahi, A., Gómez, F. A., Grand, R. J. J., Oman, K. A., Navarro, J. F., & Simpson, C. M. (2019) · arXiv · doi:10.48550/arxiv.1911.04557 · Cited by 335
STARS, GAS, AND DARK MATTER IN THE SOLAR NEIGHBORHOOD
McKee, C. F., Parravano, A., & Hollenbach, D. J. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/814/1/13 · Cited by 270 · see citing works
ON THE SHOULDERS OF GIANTS: PROPERTIES OF THE STELLAR HALO AND THE MILKY WAY MASS DISTRIBUTION
Kafle, P. R., Sharma, S., Lewis, G. F., & Bland-Hawthorn, J. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/794/1/59 · Cited by 215 · see citing works
- Authors
- Kuijken, K., & Gilmore, G.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1991-01
- Volume
- 367
- Pages
- L9
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2077809279
- Cited by
- 286
- References
- 0
- Citations by year
- 2026: 3 · 2025: 4 · 2024: 4 · 2023: 6 · 2022: 3 · 2021: 6 · 2020: 20 · 2019: 5 · 2018: 8 · 2017: 8 · 2016: 19 · 2015: 10 · 2014: 12 · 2013: 16 · 2012: 10
- FWCI
- 4.99
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astrophysical Journal (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- Galactic halo, galaxy rotation curves, disk mass, solar neighborhood
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