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- W2949270210 endingPage "2454" @default.
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- W2949270210 abstract "The ultra-diffuse dwarf galaxy NGC 1052-DF2 (DF2) has ten (eleven) measured globular clusters (GCs) with a line-of-sight velocity dispersion of $sigma=7.8^{+5.2}_{-2.2},$km/s ($sigma=10.6^{+3.9}_{-2.3},$km/s). Our conventional statistical analysis of the original ten GCs gives $sigma=8.0^{+4.3}_{-3.0},$km/s. The overall distribution of velocities agrees well with a Gaussian of this width. Due to the non-linear Poisson equation in MOND, a dwarf galaxy has weaker self-gravity when in close proximity to a massive host. This external field effect is investigated using a new analytic formulation and fully self-consistent live $N$-body models in MOND. Our formulation agrees well with that of Famaey and McGaugh (2012). These new simulations confirm our analytic results and suggest that DF2 may be in a deep-freeze state unique to MOND. The correctly calculated MOND velocity dispersion agrees with our inferred dispersion and that of van Dokkum et al. (2018b) if DF2 is within 150 kpc of NGC 1052 and both are 20 Mpc away. The GCs of DF2 are however significantly brighter and larger than normal GCs, a problem which disappears if DF2 is significantly closer to us. A distance of 10-13 Mpc makes DF2 a normal dwarf galaxy even more consistent with MOND and the 13 Mpc distance reported by Trujillo et. al. (2019). We discuss the similar dwarf DF4, finding good agreement with MOND. We also discuss possible massive galaxies near DF2 and DF4 along with their distances and peculiar velocities, noting that NGC 1052 may lie at a distance near 10 Mpc." @default.
- W2949270210 created "2019-06-27" @default.
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- W2949270210 date "2019-05-29" @default.
- W2949270210 modified "2023-10-17" @default.
- W2949270210 title "A new formulation of the external field effect in MOND and numerical simulations of ultra-diffuse dwarf galaxies – application to NGC 1052-DF2 and NGC 1052-DF4" @default.
- W2949270210 cites W11134133 @default.
- W2949270210 cites W1904244634 @default.
- W2949270210 cites W1975909368 @default.
- W2949270210 cites W1980334213 @default.
- W2949270210 cites W1990148897 @default.
- W2949270210 cites W1994959885 @default.
- W2949270210 cites W1995946163 @default.
- W2949270210 cites W2013949855 @default.
- W2949270210 cites W2014592430 @default.
- W2949270210 cites W2019292783 @default.
- W2949270210 cites W2027441044 @default.
- W2949270210 cites W2033599776 @default.
- W2949270210 cites W2034195644 @default.
- W2949270210 cites W2041542911 @default.
- W2949270210 cites W2045028470 @default.
- W2949270210 cites W2045124677 @default.
- W2949270210 cites W2050977129 @default.
- W2949270210 cites W2056131822 @default.
- W2949270210 cites W2057016204 @default.
- W2949270210 cites W2066419887 @default.
- W2949270210 cites W2077005128 @default.
- W2949270210 cites W2078353411 @default.
- W2949270210 cites W2079303893 @default.
- W2949270210 cites W2080666997 @default.
- W2949270210 cites W2087517229 @default.
- W2949270210 cites W2095433378 @default.
- W2949270210 cites W2095759197 @default.
- W2949270210 cites W2107436274 @default.
- W2949270210 cites W2131462302 @default.
- W2949270210 cites W2142220522 @default.
- W2949270210 cites W2142426937 @default.
- W2949270210 cites W2145458930 @default.
- W2949270210 cites W2160472646 @default.
- W2949270210 cites W2167073669 @default.
- W2949270210 cites W2176316361 @default.
- W2949270210 cites W2256965610 @default.
- W2949270210 cites W2293492199 @default.
- W2949270210 cites W2352435472 @default.
- W2949270210 cites W2401959413 @default.
- W2949270210 cites W2574409480 @default.
- W2949270210 cites W2610438368 @default.
- W2949270210 cites W2625830509 @default.
- W2949270210 cites W2749433822 @default.
- W2949270210 cites W2753043425 @default.
- W2949270210 cites W2789972793 @default.
- W2949270210 cites W2794449838 @default.
- W2949270210 cites W2795221662 @default.
- W2949270210 cites W2797088231 @default.
- W2949270210 cites W2797872946 @default.
- W2949270210 cites W2810718612 @default.
- W2949270210 cites W2890036657 @default.
- W2949270210 cites W2896238880 @default.
- W2949270210 cites W2898706592 @default.
- W2949270210 cites W2909449638 @default.
- W2949270210 cites W2909545561 @default.
- W2949270210 cites W2912420166 @default.
- W2949270210 cites W2912657033 @default.
- W2949270210 cites W2950236734 @default.
- W2949270210 cites W2952179566 @default.
- W2949270210 cites W3005079263 @default.
- W2949270210 cites W3083336805 @default.
- W2949270210 cites W3099270805 @default.
- W2949270210 cites W3099624329 @default.
- W2949270210 cites W3101281638 @default.
- W2949270210 cites W3101986014 @default.
- W2949270210 cites W3102713195 @default.
- W2949270210 cites W3102899763 @default.
- W2949270210 cites W3103170606 @default.
- W2949270210 cites W3103374809 @default.
- W2949270210 cites W3103572147 @default.
- W2949270210 cites W3103728112 @default.
- W2949270210 cites W3104272334 @default.
- W2949270210 cites W3106181848 @default.
- W2949270210 cites W3122068054 @default.
- W2949270210 cites W3122371004 @default.
- W2949270210 cites W3122417624 @default.
- W2949270210 cites W4244519408 @default.
- W2949270210 cites W4288360388 @default.
- W2949270210 cites W4292875581 @default.
- W2949270210 cites W4297845698 @default.
- W2949270210 cites W4298296175 @default.
- W2949270210 doi "https://doi.org/10.1093/mnras/stz1465" @default.
- W2949270210 hasPublicationYear "2019" @default.