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    <title>star formation histories | Joanna Sakowska</title>
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    <description>star formation histories</description>
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      <title>star formation histories</title>
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      <title>Unveiling the purely young star formation history of the SMC&#39;s northeastern shell from colour-magnitude diagram fitting</title>
      <link>https://joannasakowska.github.io/publication/sakowska_2024/</link>
      <pubDate>Thu, 01 Aug 2024 00:00:00 +0000</pubDate>
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      <title>Star Formation History of the Magellanic Cloud galaxies</title>
      <link>https://joannasakowska.github.io/project/sfh/</link>
      <pubDate>Wed, 27 Apr 2022 00:00:00 +0000</pubDate>
      <guid>https://joannasakowska.github.io/project/sfh/</guid>
      <description>&lt;p&gt;Visible with the naked eye, the Magellanic Cloud galaxies are our closest pair of interacting dwarf galaxies. Thus, they constitute a unique opportunity to study galactic evolution in precious detail.&lt;/p&gt;
&lt;p&gt;During my PhD thesis (&lt;a href=&#34;https://openresearch.surrey.ac.uk/esploro/outputs/doctoral/Tracing-the-Structure-and-Evolutionary-History/99918066602346&#34; target=&#34;_blank&#34; rel=&#34;noopener&#34;&gt;available here&lt;/a&gt;) I worked on the star formation and chemical evolution history of the Small Magellanic Cloud using data from the Survey of the MAgellanic Stellar History (SMASH; &lt;a href=&#34;https://ui.adsabs.harvard.edu/abs/2021AJ....161...74N/abstract&#34; target=&#34;_blank&#34; rel=&#34;noopener&#34;&gt;Nidever+2021,&lt;/a&gt; including Sakowska). I focused on a peculiar shell-like structure in the northeastern part of the galaxy, crediting its formation to interactions with the neighbouring Large Magellanic Cloud (&lt;a href=&#34;https://ui.adsabs.harvard.edu/abs/2024MNRAS.532.4272S/abstract&#34; target=&#34;_blank&#34; rel=&#34;noopener&#34;&gt;Sakowska+ 2024&lt;/a&gt;).&lt;/p&gt;
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