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brite_science [2019/02/01 15:48]
andrzej
brite_science [2019/04/05 15:49] (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: ​February 1, 2019. +   <​span style="​color:​ maroon;">​other papers.</​span></​br>​Last updated: ​April 5, 2019. 
    </​p>​    </​p>​
        
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     </​colgroup>  ​     </​colgroup>  ​
 <​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;">​ 
 +   ​179.</​span></​td>​ 
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​ 
 +   ​65.</​span></​td>​ 
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​ 
 +Walczak ​ P., Daszyńska-Daszkiewicz J., Pigulski A., Pamyatnykh A., Moffat A.F.J., Handler G., Pablo H., Popowicz A., Wade G., Weiss W.W., Zwintz K.</​span></​br>​ 
 +<span style="​color:​ black;">​Monthly Notices of the Royal Astronomical Society 485, 3544</​span>​ 
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1903.04224"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1093/​mnras/​stz639">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Seismic modelling of early B-type pulsators observed by BRITE. I. &theta; Ophiuchi</​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;">​ 
 +   ​178.</​span></​td>​ 
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​ 
 +   ​64.</​span></​td>​ 
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​ 
 +Kallinger T., Beck P.G., Hekker S., Huber D., Kuschnig R., Rockenbauer M., Winter P.M., Weiss W.W., Handler G., Moffat A.F.J., Pigulski A., Popowicz A., Wade G., Zwintz K.</​span></​br>​ 
 +<span style="​color:​ black;">​Astronomy & Astrophysics 624, A35</​span>​ 
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1902.07531"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201834514">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation</​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;">​ 
 +   ​177.</​span></​td>​ 
 +<td style="​text-align:​right"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small; color: black;">​ 
 +   ​63.</​span></​td>​ 
 +<td style="​text-align:​left"><​span style="​text-align=right;​ font-family:​ Helvetica,​Arial,​Verdana;​ font-size: small;"><​span style="​color:​ blue;">​ 
 +Schmutz W., Koenigsberger G.</​span></​br>​ 
 +<span style="​color:​ black;">​Astronomy & Astrophysics 624, L5</​span>​ 
 +<span style="​color:​ #​777777;">​ [<a href="​https://​arxiv.org/​abs/​1903.09501"​ target="​_blank">​arXiv</​a>​] [<a href="​https://​doi.org/​10.1051/​0004-6361/​201935094">​DOI</​a>​]<​br /><​span style="​font-family:​ Helvetica,​Arial;​ color: red; font-size: small;">​Long uninterrupted photometric observations of the Wolf-Rayet star EZ CMa by the Toronto BRITE satellite reveal a very fast apsidal motion</​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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 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>​ 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:​ 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 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 ​HD 149404</​span>​
 </​span>​ </​span>​
 </​td>  ​ </​td>  ​
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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.1549054107.txt.gz · Last modified: 2019/02/01 15:48 by andrzej