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Quadruple-peaked spectral line profiles as a tool to constrain gravitational potential of shell galaxies

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129335" target="_blank" >RIV/00216208:11320/12:10129335 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00387366 RIV/00216224:14310/12:00057988

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201219940" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201219940</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201219940" target="_blank" >10.1051/0004-6361/201219940</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Quadruple-peaked spectral line profiles as a tool to constrain gravitational potential of shell galaxies

  • Original language description

    Context: Stellar shells observed in many giant elliptical and lenticular as well as a few spiral and dwarf galaxies presumably result from galaxy mergers. Line-of-sight velocity distributions of the shells could, in principle, if measured with a sufficiently high signal-to-noise ratio, constitute a method to constrain the gravitational potential of the host galaxy. Aims. Merrifield & Kuijken (1998, MNRAS, 297, 1292) predicted a double-peaked line profile for stationary shells resulting from a nearly radial minor merger. In this paper, we aim at extending their analysis to a more realistic case of expanding shells, inherent to the merging process, whereas we assume the same type of merger and the same orbital geometry. Methods. We used an analytical approach as well as test particle simulations to predict the line-of-sight velocity profile across the shell structure. Simulated line profiles were convolved with spectral PSFs to estimate peak detectability. Results. The resulting line-of-

  • 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

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2012

  • 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

    545

  • Issue of the periodical within the volume

    září

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    15

  • Pages from-to

  • UT code for WoS article

    000309254900033

  • EID of the result in the Scopus database