Simulations of Line Profile Structure in Shell Galaxies

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00355557" target="_blank" >RIV/67985815:_____/10:00355557 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/10:00058551
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Simulations of Line Profile Structure in Shell Galaxies
Original language description
In the context of exploring mass distributions of dark matter haloes in giant ellipticals, we extend the analysis carried out by Merrifield & Kuijken (1998) for stellar line profiles of shells created in nearly radial mergers of galaxies. We show that line-of-sight velocity distributions are more complex than previously predicted. We simulate shell formation and analyze the detectability of spectroscopic signatures of shells after convolution with spectral PSFs.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Galaxy Wars: Stellar Populations and StarFormation in Interacting Galaxies
ISBN
978-1-58381-726-1
ISSN
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e-ISSN
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Number of pages
4
Pages from-to
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Publisher name
Astronomical Society of the Pacific
Place of publication
Melville
Event location
Johnson City
Event date
Jul 19, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000284979300045

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