The 2008 outburst in the Young Stellar System Z CMa. III - Multi-epoch high-angular resolution images and spectra of the components in near-infrared

Abstract

Z CMa is a complex pre-main sequence binary with a current separation of 100 mas, known to consist of an FU Orionis star (SE component) and an embedded Herbig Be star (NW component). Immediately when the late-2008 outburst of Z CMa was announced to the community, we initiated a high angular resolution imaging campaign with VLT/NaCo, Keck/NIRC2, VLT/SINFONI, and Keck/OSIRIS which aimed at characterizing the outburst of both components of the system in the near-infrared. We confirm that the NW star dominates the system flux in the 1.1-3.8 microns range and is responsible for the photometric outburst. We extract the first medium-resolution (R=2000-4000) near-infrared (1.1-2.4 microns) spectra of the individual components during and after the outburst. The SE component has a spectrum typical of FU Orionis objects. The NW component spectrum is characteristic of embedded outbursting protostars and EX Or objects. It displays numerous emission lines during the outburst whose intensity correlates with the system activity. In particular, we find a correlation between the Brackett gamma equivalent width and the system brightness. The bluing of the continuum of the NW component along with the absolute flux and color-variation of the system during the outburst suggests that the outburst was caused by a complex interplay between a variation of the extinction in the line of sight of the NW component on one hand, and the emission of shocked regions close to the NW component on the other. We confirm the recently reported wiggling of the SE component jet from [Fe II] line emission. We find a point-like structure associated with a peak emission at 2.098 microns coincidental with the clump or arm seen in broadband polarization differential imaging as well as additional diffuse emission along a PA=214 degrees. The origin of these two structures is unclear and deserves further investigation.

18 pages, 18 figures, 7 tables. Accepted for publication in Astronomy and Astrophysics

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Cited by in corpus (8)

• A likely flyby of binary protostar Z CMa caught in action
• The 2014-2017 outburst of the young star ASASSN-13db: A time-resolved picture of a very low-mass star between EXors and FUors
• Sustained FU Orionis-type outbursts from colliding discs in stellar flybys
• Sub-0.1" optical imaging of the Z CMa jets with SPHERE/ZIMPOL
• Spectroscopic confirmation of high-amplitude eruptive YSOs and dipping giants from the VVV survey
• CS Cha B: A disc-obscured M-type star mimicking a polarised planetary companion
• Large-Scale Ejecta of Z CMa -- Proper Motion Study and New Features Discovered
• The Effelsberg survey of FU~Orionis and EX~Lupi objects II. -- H${}_2$O maser observations