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--- bscience [2025/07/31 17:22]
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+++ bscience [2026/03/08 08:56] (current)
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    <span style="color: green;">conference papers,</span>
    <span style="color: black;">and </span>
-   <span style="color: maroon;">other papers.</span></br>Last updated: August 31, 2025.
+   <span style="color: maroon;">other papers.</span></br>Last updated: March 7, 2026.
    </p>
+<p style="font-family: Helvetica,Arial,Verdana, sans-serif; font-size: 22px; vertical-align: bottom;
+   color: #006699; text-align: center;"><strong>2026:</strong></p>
+<table style="background-color: #eeffff;" border="2" width="95%" rules="all" cellspacing="1" cellpadding="4"
+       align="center">
+    <colgroup>
+       <col span="1" style="width: 3%;">
+       <col span="1" style="width: 3%;">
+       <col span="1" style="width: 89%;">
+    </colgroup>
+<tbody>
+<tr>
+<td style="text-align:right"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size: small; color: black;">
+.</span></td>
+<td style="text-align:right"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size: small; color: black;">
+.</span></td>
+<td style="text-align:left"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size:
+small;"><span style="color: blue;">Begari T., Bernhard K., Paunzen E., Mondal P.</span></br>
+<span style="color: black;">Monthly Notices of the Royal Astronomical Society 546, 1–13<span style="color: #777777;"> [<a href="https://doi.org/10.1093/mnras/stag194" target="_blank">DOI</a>]</span><br /></span><span style="font-family:
+Helvetica,Arial; color: red; font-size: small;">Chemically peculiar stars investigated by the BRITE mission</span></span></td>
+</tr>
+<tr>
+<td style="text-align:right"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size: small; color: black;">
+.</span></td>
+<td style="text-align:right"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size: small; color: black;">
+.</span></td>
+<td style="text-align:left"><span style="text-align=right; font-family: Helvetica,Arial,Verdana; font-size:
+small;"><span style="color: blue;">Moffat A.F.J., Ignace R., Chené A.-N., Lenoir-Craig G.</span></br>
+<span style="color: black;">The Astrophysical Journal 999, 45, 1-11<span style="color: #777777;"> [<a href="https://doi.org/10.3847/1538-4357/ae3187" target="_blank">DOI</a>]</span><br /></span><span style="font-family:
+Helvetica,Arial; color: red; font-size: small;">BRITE nanosat photometry reveals bright spots in the single Wolf–Rayet star EZ CMa that can drive spectral-line-emitting corotating interaction regions</span></span></td>
+</tr>
+</tbody>
+</table>
 <p style="font-family: Helvetica,Arial,Verdana, sans-serif; font-size: 22px; vertical-align: bottom;

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