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• W2064553328 abstract "Context. Classical T Tauri stars (CTTS) differ in their X-ray signatures from older pre-main sequence stars, e.g. weaklined TTS (WTTS). CTTS show a soft excess and deviations from the low-density coronal limit in the He-like triplets. Aims. We test whether these features correlate with accretion or the presence of a disk by observing IM Lup, a diskbearing object apparently in transition between CTTS and WTTS without obvious accretion. Methods. We analyse a Chandra grating spectrum and additional XMM-Newton data of IM Lup and accompanying optical spectra, some of them taken simultaneously to the X-ray observations. We fit the X-ray emission lines and" @default.
• W2064553328 created "2016-06-24" @default.
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• W2064553328 date "2010-09-01" @default.
• W2064553328 modified "2023-09-26" @default.
• W2064553328 title "The disk-bearing young star IM Lupi - X-ray properties and limits on accretion" @default.
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