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
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Czech description
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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
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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
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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
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UT code for WoS article
000309254900033
EID of the result in the Scopus database
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