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brite_science [2018/12/21 15:09]
andrzej
brite_science [2019/03/04 09:30] (current)
andrzej
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    <​span style="​color:​ green;">​conference papers,</​span>​    <​span style="​color:​ green;">​conference papers,</​span>​
    <​span style="​color:​ black;">​and </​span>​    <​span style="​color:​ black;">​and </​span>​
-   <​span style="​color:​ maroon;">​other papers.</​span></​br>​Last updated: ​December 212018+   <​span style="​color:​ maroon;">​other papers.</​span></​br>​Last updated: ​February 12019
    </​p>​    </​p>​
        
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 <​tbody>​ <​tbody>​
 </​tr> ​ </​tr> ​
 +<​tr> ​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​176.</​span></​td>​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​62.</​span></​td>​
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​
 +Buysschaert B., Neiner C., Martin A.J., Oksala M.E., Aerts C., Tkachenko A., Alecian E., the MiMeS Collaboration</​span></​br>​
 +<span style="​color:​ black;">​Astronomy & Astrophysics 622, A67</​span>​
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1808.05503"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201731913">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Magnetic characterization and variability study of the magnetic SPB star o Lupi</​span>​
 +</​span>​
 +</​td>  ​
 +</tr>
 <​tr> ​ <​tr> ​
 <td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​ <td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
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 <td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​ <td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​
 Ramiaramanantsoa T., Ratnasingam R., Shenat T., Moffat A.F.J., Rogers T.M., Popowicz A., Kuschnig R., Pigulski A., Handler G., Wade G.A., Zwintz K., Weiss W.W.</​span></​br>​ Ramiaramanantsoa T., Ratnasingam R., Shenat T., Moffat A.F.J., Rogers T.M., Popowicz A., Kuschnig R., Pigulski A., Handler G., Wade G.A., Zwintz K., Weiss W.W.</​span></​br>​
-<span style="​color:​ black;">​Monthly Notices of the Royal Astronomical ​Observatory ​480, 972</​span>​+<span style="​color:​ black;">​Monthly Notices of the Royal Astronomical ​Society ​480, 972</​span>​
 <span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1807.04660"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1093/​mnras/​sty1897">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​A BRITE view on the massive O-type supergiant V973 Scorpii: hints towards internal gravity waves or sub-surface convection zones</​span>​ <span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1807.04660"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1093/​mnras/​sty1897">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​A BRITE view on the massive O-type supergiant V973 Scorpii: hints towards internal gravity waves or sub-surface convection zones</​span>​
 </​span>​ </​span>​
brite_science.1545422996.txt.gz ยท Last modified: 2018/12/21 15:09 by andrzej