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- W3100986175 endingPage "A46" @default.
- W3100986175 startingPage "A46" @default.
- W3100986175 abstract "Aims. We present a study of protoplanetary disks in spatially resolved low-mass binary stars in the well-known Orion nebula cluster (ONC) to assess the impact of binarity on the properties of circumstellar disks. This is currently the largest such study in a clustered high-stellar-density star-forming environment, as opposed to previous studies, which have mostly been focussed on the young, low-stellar-density Taurus association. We particularly aim to determine the presence of magnetospheric accretion and dust disks for each binary component, and measure the overall disk frequency." @default.
- W3100986175 created "2020-11-23" @default.
- W3100986175 creator A5000256641 @default.
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- W3100986175 date "2012-03-23" @default.
- W3100986175 modified "2023-10-14" @default.
- W3100986175 title "Protoplanetary disks of T Tauri binary systems in the Orion nebula cluster" @default.
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- W3100986175 doi "https://doi.org/10.1051/0004-6361/201118314" @default.
- W3100986175 hasPublicationYear "2012" @default.
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