User Tools

Site Tools


brite_science

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

brite_science [2018/09/14 14:00]
andrzej
brite_science [2019/02/01 15:48] (current)
andrzej
Line 33: Line 33:
    <​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: ​September 142018+   <​span style="​color:​ maroon;">​other papers.</​span></​br>​Last updated: ​February 12019
    </​p>​    </​p>​
 +   
 +<p style="​font-family:​ Helvetica,​Arial,​Verdana,​ sans-serif; font-size: 22px; vertical-align:​ bottom; ​
 +   ​color:​ #006699; text-align: center;"><​strong>​2019:</​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> ​
 +<​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> ​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​175.</​span></​td>​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​61.</​span></​td>​
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​
 +Rauw G., Pigulski A., Nazé Y., David-Uraz A., Handler G., Raucq F., Gosset E., Moffat A.F.J., Neiner C., Pablo H., Popowicz A., Rucinski S.M., Wade G.A., Weiss W.W., Zwintz K.</​span></​br>​
 +<span style="​color:​ black;">​Astronomy & Astrophysics 621, A15</​span>​
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1811.03306"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201833594">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​BRITE photometry of the massive post-RLOF system HD149404</​span>​
 +</​span>​
 +</​td>  ​
 +</tr>
 +</​tbody>​
 +</​table>​
 <p style="​font-family:​ Helvetica,​Arial,​Verdana,​ sans-serif; font-size: 22px; vertical-align:​ bottom; ​ <p style="​font-family:​ Helvetica,​Arial,​Verdana,​ sans-serif; font-size: 22px; vertical-align:​ bottom; ​
    ​color:​ #006699; text-align: center;"><​strong>​2018:</​strong></​p>​    ​color:​ #006699; text-align: center;"><​strong>​2018:</​strong></​p>​
Line 46: Line 84:
 <​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;">​
 +   ​174.</​span></​td>​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​60.</​span></​td>​
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​
 +Baade D., Pigulski A., Rivinius T., Wang L., Martayan C., Handler G., Panoglou D., Carciofi A.C., Kuschnig R., Mehner A., Moffat A.F.J., Pablo H., Rucinski S.M., Wade G.A., Weiss W.W., Zwintz K.</​span></​br>​
 +<span style="​color:​ black;">​Astronomy & Astrophysics 620, A145</​span>​
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1808.10254"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201834161">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Short-term variability and mass loss in Be stars. IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of &nu; Puppis (B7-8 IIIe)</​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;">​
 +   ​173.</​span></​td>​
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​
 +   ​59.</​span></​td>​
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​
 +Krtička J., Feldmeier A.</​span></​br>​
 +<span style="​color:​ black;">​Astronomy &amp; Astrophysics 617, A121</​span>​
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1807.09407"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201731614">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Light variations due to the line-driven wind instability and wind blanketing in O stars</​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;">​
brite_science.1536948023.txt.gz · Last modified: 2018/09/14 14:00 by andrzej