The top documents tagged [eclipsing binaries]

L ocating and O bserving O ptical C ounterparts to U nmodeled P ulses in Gravitational Waves LOOC UP LIGO-G070827-00-Z Dec 16, 2007 Jonah Kanner, Peter
Documents L ocating and O bserving O ptical C ounterparts to U nmodeled P ulses in Gravitational Waves LOOC UP LIGO-G070827-00-Z Dec 16, 2007 Jonah Kanner, Peter

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CoRoT fields before CoRoT – Processing of Large Photometric Databases Zoltán Csubry Konkoly Observatory Budapest, Hungary Hungarian CoRoT Day Budapest,
Documents CoRoT fields before CoRoT – Processing of Large Photometric Databases Zoltán Csubry Konkoly Observatory Budapest, Hungary Hungarian CoRoT Day Budapest,

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Observations of Binaries in Globular Clusters
Documents Observations of Binaries in Globular Clusters

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Transient Identification and Classification with WISE
Documents Transient Identification and Classification with WISE

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PTFIDE and Forced Photometry
Documents PTFIDE and Forced Photometry

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The Moon -Around the Earth and in the Sky Why do we see phases of the Moon? When do we see the phases of the Moon? What causes eclipses? Our goals for
Documents The Moon -Around the Earth and in the Sky Why do we see phases of the Moon? When do we see the phases of the Moon? What causes eclipses? Our goals for

223 views

Magdalena Ridge Observatory Interferometer
Documents Magdalena Ridge Observatory Interferometer

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Blake Head. A variable star is simply a star that changes in brightness over a set period of time (generally). This can happen in eclipsing binaries,
Documents Blake Head. A variable star is simply a star that changes in brightness over a set period of time (generally). This can happen in eclipsing binaries,

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And self enrichment of globular clusters Norbert Langer (Bonn) Onno Pols (Utrecht) Rob Izzard (Brussels) Norbert Langer (Bonn) Onno Pols (Utrecht) Rob
Documents And self enrichment of globular clusters Norbert Langer (Bonn) Onno Pols (Utrecht) Rob Izzard (Brussels) Norbert Langer (Bonn) Onno Pols (Utrecht) Rob

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CoRoT fields before CoRoT – Processing of Large Photometric Databases
Documents CoRoT fields before CoRoT – Processing of Large Photometric Databases

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(rad) = d/D = d/1AU = 0.53(2 /360 ) = 0.0093, hence d = 0.0093AU = 0.0093 x 1.496 x 10 8 km = 1.392 x 10 6 km or R sun = 6.96 x 10 5 km Can we apply
Documents (rad) = d/D = d/1AU = 0.53(2 /360 ) = 0.0093, hence d = 0.0093AU = 0.0093 x 1.496 x 10 8 km = 1.392 x 10 6 km or R sun = 6.96 x 10 5 km Can we apply

224 views

L ocating and O bserving O ptical C ounterparts to U nmodeled P ulses in Gravitational Waves
Documents L ocating and O bserving O ptical C ounterparts to U nmodeled P ulses in Gravitational Waves

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