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Testing MOND gravity in the shell galaxy NGC 3923

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10193300" target="_blank" >RIV/00216208:11320/13:10193300 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/13:00422929 RIV/00216224:14310/13:00070675

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201322060" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201322060</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201322060" target="_blank" >10.1051/0004-6361/201322060</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Testing MOND gravity in the shell galaxy NGC 3923

  • Original language description

    Context. The elliptical galaxy NGC3923 is surrounded by numerous stellar shells that are concentric arcs centered on the Galactic core. They are very likely a result of a minor merger and they consist of stars in nearly radial orbits. For a given potential, the shell radii at a given time after the merger can be calculated and compared to observations. The MOdified Newtonian Dynamics (MOND) is a theory that aims to solve the missing mass problem by modifying the laws of classical dynamics in the limit of small accelerations. Hernquist & Quinn (1987b, ApJ, 312, 1) claimed that the shell distribution of NGC3923 contradicted MOND, but Milgrom (1988, ApJ, 332, 86) found several substantial insufficiencies in their work. Aims. We test whether the observed shell distribution in NGC3923 is consistent with MOND using the current observational knowledge of the shell number and positions and of the host galaxy surface brightness profile, which supersede the data available in the 1980s when the l

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2013

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    559

  • Issue of the periodical within the volume

    listopad

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    8

  • Pages from-to

  • UT code for WoS article

    000327847200110

  • EID of the result in the Scopus database