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dc.contributor.authorHaghi, Hosein
dc.contributor.authorKroupa, Pavel
dc.contributor.authorBanik, Indranil
dc.contributor.authorWu, Xufen
dc.contributor.authorZonoozi, Akram Hasani
dc.contributor.authorJavanmardi, Behnam
dc.contributor.authorGhari, Amir
dc.contributor.authorMueller, Oliver
dc.contributor.authorDabringhausen, Joerg
dc.contributor.authorZhao, Hongsheng
dc.date.accessioned2019-07-25T09:30:05Z
dc.date.available2019-07-25T09:30:05Z
dc.date.issued2019-08
dc.identifier.citationHaghi , H , Kroupa , P , Banik , I , Wu , X , Zonoozi , A H , Javanmardi , B , Ghari , A , Mueller , O , Dabringhausen , J & Zhao , H 2019 , ' 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 ' , Monthly Notices of the Royal Astronomical Society , vol. 487 , no. 2 , pp. 2441-2454 . https://doi.org/10.1093/mnras/stz1465en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 260290416
dc.identifier.otherPURE UUID: 72e888d9-ed10-492b-90ae-062c291477c9
dc.identifier.otherWOS: 000474919700068
dc.identifier.otherORCID: /0000-0002-4123-7325/work/59953718
dc.identifier.otherWOS: 000474919700068
dc.identifier.otherScopus: 85071133469
dc.identifier.urihttp://hdl.handle.net/10023/18162
dc.descriptionOM thanks the Swiss National Science Foundation for financial support. XW gives thanks for support from the Natural Science Foundation of China grants numbers 11503025 and 11421303, Anhui Natural Science Foundation grant number 1708085MA20 and the ‘Hundred Talents Project of Anhui Province’.en
dc.description.abstractThe ultra-diffuse dwarf galaxy NGC 1052-DF2 (DF2) has 10 (11) measured globular clusters (GCs) with a line-of-sight velocity dispersion of σ=7.8+5.2−2.2 km s−1 (⁠σ=10.6+3.9−2.3 km s−1). Our conventional statistical analysis of the original 10 GCs gives σ=8.0+4.3−3.0 km s−1. 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. 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. 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.. 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.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsCopyright © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. his work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://doi.org/10.1093/mnras/stz1465en
dc.subjectGravitationen
dc.subjectGalaxies: distances and redshiftsen
dc.subjectGalaxies: dwarfen
dc.subjectGalaxies: individual: NGC 1052-DF2en
dc.subjectGalaxies: kinematics and dynamicsen
dc.subjectDark matteren
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleA 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-DF4en
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stz1465
dc.description.statusPeer revieweden


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