Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33
Abstract: We have developed a fast numerical 2-D model of galaxy disk evolution (resolved along the galaxy radius and azimuth) by adopting a scheme of parameterized stochastic self-propagating star formation. We explore the parameter space of the model and demonstrate its capability to reproduce 1-D radial profiles of the galaxy M33: gas surface density, surface brightness in the i and GALEX FUV passbands, and metallicity.
- Standort
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Deutsche Nationalbibliothek Frankfurt am Main
- Umfang
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Online-Ressource
- Sprache
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Englisch
- Erschienen in
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Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33 ; volume:23 ; number:3-4 ; year:2014 ; pages:209-220 ; extent:12
Open astronomy ; 23, Heft 3-4 (2014), 209-220 (gesamt 12)
- Urheber
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Mineikis, T.
Vansevičius, V.
- DOI
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10.1515/astro-2017-0183
- URN
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urn:nbn:de:101:1-2405271659450.245258447898
- Rechteinformation
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Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
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14.08.2025, 11:00 MESZ
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Beteiligte
- Mineikis, T.
- Vansevičius, V.
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