Hydrodynamic simulations of the triaxial bulge of M 31
Citations
737 citations
Cites background from "Hydrodynamic simulations of the tri..."
...Those anomalies are attributed to the presence of a triaxial bar/bulge in M31 (e.g. Stark 1977; Stark & Binney 1994; Berman 2001)....
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198 citations
Cites background from "Hydrodynamic simulations of the tri..."
...The location of these spots and appearance of the nuclear region (especially at 70 µm) is similar to the triaxial bulge simulations of Berman (2001)....
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193 citations
Cites background from "Hydrodynamic simulations of the tri..."
...Its non-circular orbit may be caused by the central bar (Berman 2001; Berman & Loinard 2002)....
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175 citations
Cites background from "Hydrodynamic simulations of the tri..."
...However, notice that this is shown not just to point out the consistency of the molecular and atomic gas velocities, but to emphasize one has to consider non-circular motion to properly trace the rotation curve in the inner region (Berman 2001; Berman & Loinard 2002)....
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...In particular Berman (2001); Berman & Loinard (2002) have shown that the anomalous velocities observed in the inner region of M31 can be explained as the response of the gas to the potential of a triaxial rotating bulge....
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...Detailed modelling of the surface brightness shows that at very least the bulge is an obl te spheroid with axis ratio of 0.8 (Kent 1983) but most likely it is a triaxial bulge (e.g. Berman 2001, and references therein)....
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...Hydrodynamic simulations of the triaxial bulge of M31 by Berman (2001) found a B-band mass-to-light ratio of 6.5 for the bulge i.e. a stellar mass of 1010 M⊙....
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References
285 citations
244 citations
"Hydrodynamic simulations of the tri..." refers background in this paper
...TheB-band surface brightness profile of the bulge of M31 follows ther 1 4 law of de Vaucouleurs (1958): I(s) = Ie exp(−7.67[(s/re) 14 − 1]) , wherere is the effective radius,Ie is the surface brightness at re ands is the semi-major axis length of the isophote....
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215 citations
"Hydrodynamic simulations of the tri..." refers background in this paper
...Using stellar kinematic data, Kormendy and Illingworth (1982) provide evidence that many SA bulges (in unbarred galaxies) are rotationally flattened, and consistent with being oblate spheroids....
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205 citations
"Hydrodynamic simulations of the tri..." refers background in this paper
...Many rotation curves can be fitted by models ranging from zero-mass disks to ‘maximum disks’ (van Albada and Sancisi 1986), that is disks that are as massive as possible whilst ensuring that the halo is not hollow....
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