Autor:
Boffin, H.M.J.
Jones, D.
Wesson, R.
Beletsky, Y.
Miszalski, B.
Saviane, I.
Monaco, L.
Corradi, R.
Santander García, M.
Rodríguez-Gil, P.
Bipolar planetary nebulae (PNe) are thought to result from binary star interactions and, indeed, tens of binary central stars of PNe have been found, in particular using photometric time-series that allow for the detection of post-common envelope systems. Using photometry at the NTT in La Silla w...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/11525
Boffin, H.M.J.
,
Jones, D.
,
Wesson, R.
,
Beletsky, Y.
,
Miszalski, B.
,
Saviane, I.
,
Monaco, L.
,
Corradi, R.
,
Santander García, M.
,
Rodríguez-Gil, P.
,
[When nature tries to trick us: An eclipsing eccentric close binary superposed on the central star of the planetary nebula M 3-2]
,
When nature tries to trick us: An eclipsing eccentric close binary superposed on the central star of the planetary nebula M 3-2
