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S. V. van Terwisga

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Open access Sep 2026

The effect of X-ray and accretion variability on mid-infrared lines in the young disk-bearing binary DQ Tau

A star's radiation field is the main energy source of a planet-forming disk. Stellar photons -- from X-rays to optical -- are reprocessed in the inner protoplanetary disk, and this process enables mid-infrared (mid-IR) diagnostics of the disk's physical conditions. Most pre-main-sequence stars accrete at moderate rates...

B. Portilla-Revelo, K. Getman, Á. Kóspál et al. · 0 citations
Review Open access Sep 2026

X-shooter survey Across Regions and Ages to probe Disk Evolution (ARADE). Accretion properties in Orion A and their relation with disk masses

We present the largest homogeneous VLT/X-shooter study of accretion in young stellar objects spanning the entire Orion A complex. Our sample includes 91 pre-main-sequence stars hosting a protoplanetary disk according to photometry, selected to span a wide range of optical colors, 34 of which have complementary ALMA dus...

L. Piscarreta, G. Beccari, C. Manara et al. · 0 citations

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