Elliptical Galaxies in MOND

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F20%3A10423658" target="_blank" >RIV/00216208:11320/20:10423658 - isvavai.cz</a>
Result on the web
<a href="https://www.mff.cuni.cz/veda/konference/wds/proc/pdf20/WDS20_05_f1_Eappen.pdf" target="_blank" >https://www.mff.cuni.cz/veda/konference/wds/proc/pdf20/WDS20_05_f1_Eappen.pdf</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Elliptical Galaxies in MOND
Original language description
Fully self-consistent simulations of the formation of elliptical galaxies in the early Universe are performed assuming no dark matter. We start with a post-Big Bang pre-galactic gas cloud, allow it to collapse under self-gravity thereby following the star formation history and chemical enrichment. Phantom of Ramses (POR) is a customized version of RAMSES and includes all its features but uses Milgromian dynamics. We compare these theoretical results with the empirical downsizing results obtained previously to infer the allowed initial conditions, given the observed properties of elliptical galaxies.
Czech name
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Czech description
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Project
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Continuities
S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
WDS'20 Proceedings of Contributed Papers — Physics
ISBN
978-80-7378-435-5
ISSN
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e-ISSN
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Number of pages
7
Pages from-to
38-44
Publisher name
Matfyzpress
Place of publication
Praha
Event location
Praha/ZOOM
Event date
Sep 22, 2020
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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