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- W2991451002 abstract "We present new X-ray observations of the optically-obscured protostar HL Tau and the intermediate mass Herbig Be star HD 100546. Both objects are surrounded by spectacular disks showing complex morphology including rings and gaps that may have been sculpted by protoplanets. HL Tau was detected as a variable hard X-ray source by Chandra, typical of late-type magnetically-active coronal sources. No extended X-ray emission was seen along the HL Tau jet, or along the jet of the T Tauri binary system XZ Tau located 23 arcsecs to its east. In contrast, HD 100546 was detected by XMM-Newton as a soft X-ray source with no short-term ( 1 au are well-shielded from X-rays produced by the central star." @default.
- W2991451002 created "2019-12-05" @default.
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- W2991451002 date "2019-11-25" @default.
- W2991451002 modified "2023-10-18" @default.
- W2991451002 title "X-ray Emission and Disk Irradiation of HL Tau and HD 100546" @default.
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