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1by Donati, J. -F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, Andrew Collier, Jardine, Moira Mary, Walker, G. A. H.Subjects: “...GIANT PLANETS...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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2by Donati, J. -F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, Andrew Collier, Jardine, Moira Mary, Walker, G. A. H.Subjects: “...GIANT PLANETS...”
Published in Monthly Notices of the Royal Astronomical Society (2008)
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3by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental, it suggests...”
Published 2008
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4by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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5by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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6by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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7by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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8by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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9by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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10by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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11by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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12by Donati, J. F., Moutou, C., Fares, R., Bohlender, D., Catala, C., Deleuil, M., Shkolnik, E., Cameron, A. C., Jardine, M. M., Walker, G. A. H.“... motion of its giant planet (period 3.3 d). Assuming that this synchronisation is not coincidental...”
Published 2008
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13by Fares, R., Donati, J. -F., Moutou, C., Jardine, M. M., Griessmeier, J. -M., Zarka, P., Shkolnik, E. L., Bohlender, D., Catala, C., Cameron, A. C.“...HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study...”
Published 2010
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14by Fares, R., Donati, J.-F., Moutou, C., Jardine, M. M., Grießmeier, J.-M., Zarka, P., Shkolnik, E. L., Bohlender, D., Catala, C., Cameron, A. C.“...HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study...”
Published in Monthly Notices of the Royal Astronomical Society (2010)
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15by Fares, R., Moutou, C., Donati, J. -F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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16by Fares, R., Moutou, C., Donati, J.-F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... magnetic field properties in the mass–rotation diagram. The comparison shows that these giant planet-host...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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17by Fares, R., Moutou, C., Donati, J. -F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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18by Fares, R., Moutou, C., Donati, J. -F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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19by Fares, R., Moutou, C., Donati, J. -F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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20by Fares, R., Moutou, C., Donati, J. -F., Catala, C., Shkolnik, E. L., Jardine, M. M., Cameron, A. C., Deleuil, M.“... that these giant planet-host stars tend to have similar magnetic field topologies to stars without detected hot...”
Published in Monthly Notices of the Royal Astronomical Society (2013)
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