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MOND prediction of a new giant shell in the elliptical galaxy NGC 3923

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00076851" target="_blank" >RIV/00216224:14310/14:00076851 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/14:00434216

  • Result on the web

    <a href="http://adsabs.harvard.edu/abs/2014A%26A...566A.151B" target="_blank" >http://adsabs.harvard.edu/abs/2014A%26A...566A.151B</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201423935" target="_blank" >10.1051/0004-6361/201423935</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    MOND prediction of a new giant shell in the elliptical galaxy NGC 3923

  • Original language description

    Context. Stellar shells, which form axially symmetric systems of arcs in some elliptical galaxies, are most likely remnants of radial minor mergers. They are observed up a radius of similar to 100 kpc. The stars in them oscillate in radial orbits. The radius of a shell depends on the free-fall time at the position of the shell and on the time since the merger. We previously verified the consistency of shell radii in the elliptical galaxy NGC 3923 with its most probable MOND potential. Our results implied that an as yet undiscovered shell exists at the outskirts of the galaxy. Aims. We here extend our study by assuming more general models for the gravitational potential to verify the prediction of the new shell and to estimate its position. Methods. Wetested the consistency of the shell radial distribution observed in NGC 3923 with a wide variety of MOND potentials of the galaxy. The potentials differed in the mass-to-light ratio and in distance to the galaxy.

  • 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

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    ASTRONOMY & ASTROPHYSICS

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    566

  • Issue of the periodical within the volume

    JUNE

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    11

  • Pages from-to

    "nestránkováno"

  • UT code for WoS article

    000338681500154

  • EID of the result in the Scopus database