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brite_science [2019/02/01 15:48]
andrzej
brite_science [2019/03/04 09:30] (current)
andrzej
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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.txt ยท Last modified: 2019/03/04 09:30 by andrzej