https://www.scipedia.com/wd/index.php?action=history&feed=atom&title=Pena_et_al_1994a 2026-04-18T02:32:11Z Revision history for this page on the wiki MediaWiki 1.27.0-wmf.10 https://www.scipedia.com/wd/index.php?title=Pena_et_al_1994a&diff=330545&oldid=prev 2026-04-07T19:22:07Z

<p>Oyam moved page <a href="/public/Draft_Gamboa_709520515" class="mw-redirect" title="Draft Gamboa 709520515">Draft Gamboa 709520515</a> to <a href="/public/Pena_et_al_1994a" title="Pena et al 1994a">Pena et al 1994a</a></p> <table class="diff diff-contentalign-left" data-mw="interface"> <tr style='vertical-align: top;' lang='en'> <td colspan='1' style="background-color: white; color:black; text-align: center;">← Older revision</td> <td colspan='1' style="background-color: white; color:black; text-align: center;">Revision as of 19:22, 7 April 2026</td> </tr><tr><td colspan='2' style='text-align: center;' lang='en'><div class="mw-diff-empty">(No difference)</div> </td></tr></table>

Oyam https://www.scipedia.com/wd/index.php?title=Pena_et_al_1994a&diff=330544&oldid=prev 2026-04-07T19:21:58Z

<p>Created page with &quot; == Abstract == &lt;p&gt;&lt;span style=&quot;color: rgb(93, 93, 93); font-size: 16px; font-style: normal; font-weight: 400;&quot;&gt;uvby-β photoelectric photometry of the open cluster NGC 1...&quot;</p> <p><b>New page</b></p><div><br /> == Abstract ==<br /> <br /> &lt;p&gt;&lt;span style=&quot;color: rgb(93, 93, 93); font-size: 16px; font-style: normal; font-weight: 400;&quot;&gt;uvby-&amp;beta; photoelectric photometry of the open cluster NGC 1342 is presented. From the analysis of photometric data reddening, distance, temperature and gravity are determined for each star, and from the distance and reddening of each, a mean distance modulus and reddening of 8.62&amp;plusmn;0.22 mag and E(b-y) = 0.297&amp;plusmn;0.112, respectively, to the cluster is assigned. An age of 4.0&amp;times;10&lt;/span&gt;&lt;span style=&quot;font-size: 12px; color: rgb(93, 93, 93); font-style: normal; font-weight: 400;&quot;&gt;8&lt;/span&gt;&lt;span style=&quot;color: rgb(93, 93, 93); font-size: 16px; font-style: normal; font-weight: 400;&quot;&gt;yr is determined through direct comparison with theoretical models. Five stars were identified in the direction of NGC 1342 as chemically peculiar stars of which four are cluster members.&lt;/span&gt;&lt;/p&gt;<br /> <br /> <br /> <br /> == Document ==<br /> &lt;pdf&gt;Media:Draft_Gamboa_709520515-8082-document.pdf&lt;/pdf&gt;</div>

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