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Chemical Signatures of the FU Ori Outbursts
Tamara Molyarova, Vitaly Akimkin, Dmitry Semenov +5
The FU Ori-type young stellar objects are characterized by a sudden increase in luminosity by 12 orders of magnitude, followed by slow return to the pre-outburst state on timesc…
Near-Infrared High-Resolution Imaging Polarimetry of FU Ori-Type Objects: Towards A Unified Scheme for Low-Mass Protostellar Evolution
Michihiro Takami, Guangwei Fu, Hauyu Baobab Liu +14
We present near-IR imaging polarimetry of five classical FU Ori-type objects (FU Ori, V1057 Cyg, V1515 Cyg, V1735 Cyg, Z CMa) with a 0\farcs1 resolution observed using HiCIAO…
Spots, flares, accretion, and obscuration in the pre-main sequence binary DQ Tau
Á. Kóspál, P. Ábrahám, G. Zsidi +4
DQ Tau is a young low-mass spectroscopic binary, consisting of two almost equal-mass stars on a 15.8 d period surrounded by a circumbinary disk. Here, we analyze DQ Tau's light cur…
VLTI/MIDI atlas of disks around low- and intermediate-mass young stellar objects
J. Varga, P. Ábrahám, L. Chen +13
Context. Protoplanetary disks show large diversity regarding their morphology and dust composition. With mid-infrared interferometry the thermal emission of disks can be spatially…