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The Young Binary DQ Tau Produces Another X-ray Flare Near Periastron
- Source :
- Research Notes of the AAS, Volume 6, Issue 3, id.64 (2022)
- Publication Year :
- 2022
-
Abstract
- This work is part of a multi-wavelength program to study the effects of X-ray/UV/optical stellar radiation on the chemistry of the circumbinary disk around the young high-eccentricity binary DQ Tau. ALMA observations for near/around December 5, 2021 periastron were postponed due to bad weather, but supporting Swift-XRT-UVOT TOO observations were successful. These Swift observations along with previous X-ray-optical-mm data show that DQ Tau keeps exhibiting powerful flares near periastron, offering a unique laboratory for studies of flare effects on the gas-phase ion chemistry in protoplanetary disks.<br />Comment: 6 pages, 1 figure, 1 table, accepted for publication in RNAAS
Details
- Database :
- arXiv
- Journal :
- Research Notes of the AAS, Volume 6, Issue 3, id.64 (2022)
- Publication Type :
- Report
- Accession number :
- edsarx.2204.01824
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.3847/2515-5172/ac618a