Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
We improved the stochastic 2-D galaxy disk models (Mineikis & Vansevičius 2014a) by introducing enriched gas outflows from galaxies and synthetic color-magnitude diagrams of stellar populations. To test the models, we use the HST/ACS stellar photometry data in four fields located along the major...
Main Authors: | , |
---|---|
Format: | Article |
Language: | English |
Published: |
De Gruyter
2015-09-01
|
Series: | Open Astronomy |
Subjects: | |
Online Access: | https://doi.org/10.1515/astro-2017-0223 |
_version_ | 1818578491098005504 |
---|---|
author | Mineikis T. Vansevičius V. |
author_facet | Mineikis T. Vansevičius V. |
author_sort | Mineikis T. |
collection | DOAJ |
description | We improved the stochastic 2-D galaxy disk models (Mineikis & Vansevičius 2014a) by introducing enriched gas outflows from galaxies and synthetic color-magnitude diagrams of stellar populations. To test the models, we use the HST/ACS stellar photometry data in four fields located along the major axis of the galaxy M33 (Williams et al. 2009) and demonstrate the potential of the models to derive 2-D star formation histories in the resolved disk galaxies. |
first_indexed | 2024-12-16T06:46:39Z |
format | Article |
id | doaj.art-7e9191201425474cbe456d351e04bd99 |
institution | Directory Open Access Journal |
issn | 2543-6376 |
language | English |
last_indexed | 2024-12-16T06:46:39Z |
publishDate | 2015-09-01 |
publisher | De Gruyter |
record_format | Article |
series | Open Astronomy |
spelling | doaj.art-7e9191201425474cbe456d351e04bd992022-12-21T22:40:31ZengDe GruyterOpen Astronomy2543-63762015-09-0124322323010.1515/astro-2017-0223astro-2017-0223Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33Mineikis T.0Vansevičius V.1 Vilnius University Observatory, Čiurlionio 29, Vilnius LT-03100, Lithuania Vilnius University Observatory, Čiurlionio 29, Vilnius LT-03100, LithuaniaWe improved the stochastic 2-D galaxy disk models (Mineikis & Vansevičius 2014a) by introducing enriched gas outflows from galaxies and synthetic color-magnitude diagrams of stellar populations. To test the models, we use the HST/ACS stellar photometry data in four fields located along the major axis of the galaxy M33 (Williams et al. 2009) and demonstrate the potential of the models to derive 2-D star formation histories in the resolved disk galaxies.https://doi.org/10.1515/astro-2017-0223galaxies: evolutiongalaxies: individual (m33) |
spellingShingle | Mineikis T. Vansevičius V. Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 Open Astronomy galaxies: evolution galaxies: individual (m33) |
title | Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 |
title_full | Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 |
title_fullStr | Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 |
title_full_unstemmed | Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 |
title_short | Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33 |
title_sort | stochastic 2 d galaxy disk evolution models resolved stellar populations in the galaxy m33 |
topic | galaxies: evolution galaxies: individual (m33) |
url | https://doi.org/10.1515/astro-2017-0223 |
work_keys_str_mv | AT mineikist stochastic2dgalaxydiskevolutionmodelsresolvedstellarpopulationsinthegalaxym33 AT vanseviciusv stochastic2dgalaxydiskevolutionmodelsresolvedstellarpopulationsinthegalaxym33 |