Počet záznamů: 1  

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

  1. 1.
    SYSNO ASEP0434216
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevMOND prediction of a new giant shell in the elliptical galaxy NGC 3923
    Tvůrce(i) Bílek, Michal (ASU-R) ORCID
    Bartošková, Kateřina (ASU-R)
    Ebrová, Ivana (ASU-R)
    Jungwiert, Bruno (ASU-R) ORCID, RID
    Zdroj.dok.Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 566, June (2014), A151/1-A151/11
    Poč.str.11 s.
    Forma vydáníTištěná - P
    Jazyk dok.eng - angličtina
    Země vyd.FR - Francie
    Klíč. slovagravitation ; galaxies: kinematics and dynamics ; galaxies: formation
    Vědní obor RIVBN - Astronomie a nebeská mechanika, astrofyzika
    Institucionální podporaASU-R - RVO:67985815
    UT WOS000338681500154
    DOI10.1051/0004-6361/201423935
    AnotaceWe 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. We tested 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. We considered different MOND interpolation functions, values of the acceleration constant a(0), and density profiles of the galaxy. We verified the functionality of our code on a Newtonian self-consistent simulation of the formation of a shell galaxy. Our method reliably predicts that exactly one new outermost shell exists at a galactocentric radius of about 1900 '' (similar to 210 kpc) on the southwestern side of the galaxy. Its estimated surface brightness is about 28 mag arcsec(-2) in B - a value accessible by current instruments. This prediction enables a rare test of MOND in an elliptical down to an acceleration of a(0)/10. The predictive power of our method is verified by reconstructing the position of the largest known shell from the distribution of the remaining shells.
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2015
Počet záznamů: 1  

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