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      <title>Stellar Clusters by هدى طه صبرى ابراهيم</title>
      <link>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv</link>
      <description></description>
      <language>en-us</language>
      <pubDate>2024-05-11 23:52:39 UTC</pubDate>
      <lastBuildDate>2024-05-12 05:30:48 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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         <title>Group 3 shereen ashraf </title>
         <author></author>
         <link>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140377</link>
         <description><![CDATA[<p>Galaxies show us how the matter in the universe is organized on large scales. In order to understand the nature and history of the universe, scientists study how the matter is currently organized and how that organization has changed through out cosmic time.</p>]]></description>
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         <pubDate>2024-05-12 05:29:12 UTC</pubDate>
         <guid>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140377</guid>
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         <title>Group 2 Nada Zain </title>
         <author></author>
         <link>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140727</link>
         <description><![CDATA[<p>There are three main types of star clusters: globular clusters, open clusters, and stellar associations, each of which has different properties that provide different information to astronomers.</p>]]></description>
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         <pubDate>2024-05-12 05:30:48 UTC</pubDate>
         <guid>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140727</guid>
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         <title>GROUP 1 :ABDELRAHMAN HESHAM </title>
         <author>abdohesham200314</author>
         <link>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140735</link>
         <description><![CDATA[<p><strong>Star Birth:</strong></p><p><br/></p><ul><li><p>Galaxies provide the essential ingredients for star formation: vast clouds of dust and gas. These clouds condense under their own gravity, eventually igniting nuclear fusion and birthing new stars.</p></li></ul><p><strong>Galactic Evolution:</strong></p><ul><li><p>Stars, in turn, shape the galaxy's structure and evolution. Stellar explosions (supernovae) can trigger the formation of new stars by compressing surrounding gas clouds. Additionally, the heavy elements forged within stars enrich the interstellar medium, influencing future generations of stars.</p></li></ul><p><strong>Galactic Interactions:</strong></p><ul><li><p>When galaxies get close enough, their gravity interacts. This can be a gentle dance or a violent collision. Even close flybys can warp galactic disks and trigger bursts of star formation due to gas compression.</p></li><li><p>Major mergers of galaxies can completely reshape them, creating elliptical galaxies or fueling extreme starburst events.</p></li></ul><p><strong>Overall Impact:</strong></p><ul><li><p>The interplay between stars and galaxies is a continuous cycle. Stars are born from galactic material, and in their lifespans and deaths, they influence the formation of new stars and the overall structure of the galaxy. This cycle has been shaping the universe since its earliest dayspen_spark</p></li></ul><p>tuneshare</p><p>more_vert"</p>]]></description>
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         <pubDate>2024-05-12 05:30:50 UTC</pubDate>
         <guid>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140735</guid>
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         <title>Group 5 rawan mohamed</title>
         <author></author>
         <link>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140905</link>
         <description><![CDATA[<p><strong>Galaxy mergers</strong> can occur when two (or more) <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Galaxy">galaxies</a> collide. They are the most violent type of <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Interacting_galaxy">galaxy interaction</a>. The <a rel="noopener noreferrer nofollow" class="mw-redirect" href="https://en.m.wikipedia.org/wiki/Gravitation">gravitational interactions</a> between galaxies and the friction between the <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Gas">gas</a> and <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Cosmic_dust">dust</a> have major effects on the galaxies involved, but the exact effects of such mergers depend on a wide variety of parameters such as <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Collision">collision</a> angles, <a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Speed">speeds</a>, and relative size/composition, and are currently an extremely active area of research. Galaxy mergers are important because the merger rate is a fundamental measurement of <a rel="noopener noreferrer nofollow" class="mw-redirect" href="https://en.m.wikipedia.org/wiki/Galaxy_evolution">galaxy evolution</a> and also provides astronomers with clues about how galaxies grew into their current forms over long stretches of time.<a rel="noopener noreferrer nofollow" href="https://en.m.wikipedia.org/wiki/Galaxy_merger#cite_note-Galaxy_Collision_Rate-1"><sup>[1]</sup></a></p>]]></description>
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         <pubDate>2024-05-12 05:31:27 UTC</pubDate>
         <guid>https://padlet.com/stembiology2023_13/v3je7fpflhnh23mv/wish/2989140905</guid>
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