The DOI matches its Crossref record; 14 of the 14 references it cites were found in a registry or an index.
The extended rotation curve and the dark matter halo of M33
Open accessAbstract
We present the 21-cm rotation curve of the nearby galaxy M33 out to a galactocentric distance of 16 kpc (13 disc scalelengths). The rotation curve keeps rising out to the last measured point and implies a dark halo mass ≳5×1010 M⊙. The stellar and gaseous discs provide virtually equal contributions to the galaxy gravitational potential at large galactocentric radii, but no obvious correlation is found between the radial distribution of dark matter and the distribution of stars or gas. Results of the best fit to the mass distribution in M33 picture a dark halo which controls the gravitational potential from 3 kpc outward, with a matter density which decreases radially as R−1.3. The density profile is consistent with the theoretical predictions for structure formation in hierarchical clustering cold dark matter (CDM) models, and favours lower mass concentrations than those expected in the standard cosmogony.
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Citations
Cites
A Universal Density Profile from Hierarchical Clustering
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On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 1×
“From the rotation curve and from the H i+He surface density, we can derive the classical disk stability parameter Q (Toomre 1964, Kennicutt 1989).”
MethodRubin, V. C., Thonnard, N., & Ford, W. K., Jr. (1980) · The Astrophysical Journal · doi:10.1086/158003 · Cited by 1,692
The star formation law in galactic disks
Kennicutt, R. C., Jr. (1989) · The Astrophysical Journal · doi:10.1086/167834 · Cited by 1,605
Third Reference Catalogue of Bright Galaxies: Volume III
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The universal rotation curve of spiral galaxies — I. The dark matter connection
Persic, M., Salucci, P., & Stel, F. (1996) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/278.1.27 · Cited by 1,238
Self-citationAdaptive Refinement Tree: A New High‐Resolution N‐Body Code for Cosmological Simulations
Kravtsov, A. V., Klypin, A. A., & Khokhlov, A. M. (1997) · The Astrophysical Journal Supplement Series · doi:10.1086/313015 · Cited by 669
Bosma, A. (1981) · The Astronomical Journal · doi:10.1086/113062 · Cited by 363
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Cited by
Beyond the Bulge: A Fundamental Relation between Supermassive Black Holes and Dark Matter Halos
Ferrarese, L. (2002) · The Astrophysical Journal · doi:10.1086/342308 · Cited by 600
The cored distribution of dark matter in spiral galaxies
Gentile, G., Salucci, P., Klein, U., Vergani, D., & Kalberla, P. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.07836.x · Cited by 579
Self-citationTHE M31 VELOCITY VECTOR. II. RADIAL ORBIT TOWARD THE MILKY WAY AND IMPLIED LOCAL GROUP MASS
van der Marel, R. P., Fardal, M., Besla, G., Beaton, R. L., Sohn, S. T., Anderson, J., Brown, T., & Guhathakurta, P. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/753/1/8 · Cited by 259
A GLOBAL STAR-FORMING EPISODE IN M31 2–4 GYR AGO
Williams, B. F., Dalcanton, J. J., Dolphin, A. E., Weisz, D. R., Lewis, A. R., Lang, D., Bell, E. F., Boyer, M., Fouesneau, M., Gilbert, K. M., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/48 · Cited by 41
The Karl G. Jansky Very Large Array Local Group L -Band Survey (LGLBS)
Koch, E. W., Leroy, A. K., Rosolowsky, E. W., Chomiuk, L., Dalcanton, J. J., Pingel, N. M., Sarbadhicary, S. K., Stanimirović, S., Walter, F., Archer, H. N., et al. (2025) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ade0ad · Cited by 13
Metadata
- Authors
- Corbelli, E., & Salucci, P.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2000-01-15
- Volume
- 311
- Issue
- 2
- Pages
- 441-447
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2118508340
- Cited by
- 386
- References
- 14
- FWCI
- 5.93
- Type
- journal article
- Language
- en
- Open access
- green
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