Chemical Signatures of the FU Ori Outbursts

Tamara Molyarova, Vitaly Akimkin, Dmitry Semenov, P. Ábrahám, Thomas Henning, Agnes Kóspál, Eduard Vorobyov, Dmitri Wiebe

Research output: Article

3 Citations (Scopus)

Abstract

The FU Ori-type young stellar objects are characterized by a sudden increase in luminosity by 1-2 orders of magnitude followed by a slow return to the pre-outburst state on timescales of ∼10-100 yr. The outburst strongly affects the entire disk, changing its thermal structure and radiation field. In this paper, using a detailed physical-chemical model, we study the impact of the FU Ori outburst on the disk chemical inventory. Our main goal is to identify gas-phase molecular tracers of the outburst activity that could be observed after the outburst with modern telescopes such as ALMA and NOEMA. We find that the majority of molecules experience a considerable increase in total disk gas-phase abundances due to the outburst, mainly due to the sublimation of their ices. Their return to the pre-outburst chemical state takes different amounts of time, from nearly instantaneous to very long. Among the former, we identify CO, NH3, C2H6, C3H4, etc. Their abundance evolution tightly follows the luminosity curve. For CO, the abundance increase does not exceed an order of magnitude, while for other tracers, the abundances increase by 2-5 orders of magnitude. Other molecules, like H2CO and NH2OH, have longer retention timescales, remaining in the gas phase for ∼10-103 yr after the end of the outburst. Thus, H2CO could be used as an indicator of the previous outbursts in the post-outburst FU Ori systems. We investigate the corresponding time-dependent chemistry in detail and present the most favorable transitions and ALMA configurations for future observations.

Original languageEnglish
Article number46
JournalAstrophysical Journal
Volume866
Issue number1
DOIs
Publication statusPublished - okt. 10 2018

Fingerprint

outburst
signatures
vapor phases
tracers
luminosity
sublimation
radiation distribution
molecules
ice
telescopes
chemistry
tracer
gas
chemical
timescale
curves
configurations
thermal structure

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Molyarova, T., Akimkin, V., Semenov, D., Ábrahám, P., Henning, T., Kóspál, A., ... Wiebe, D. (2018). Chemical Signatures of the FU Ori Outbursts. Astrophysical Journal, 866(1), [46]. https://doi.org/10.3847/1538-4357/aadfd9

Chemical Signatures of the FU Ori Outbursts. / Molyarova, Tamara; Akimkin, Vitaly; Semenov, Dmitry; Ábrahám, P.; Henning, Thomas; Kóspál, Agnes; Vorobyov, Eduard; Wiebe, Dmitri.

In: Astrophysical Journal, Vol. 866, No. 1, 46, 10.10.2018.

Research output: Article

Molyarova, T, Akimkin, V, Semenov, D, Ábrahám, P, Henning, T, Kóspál, A, Vorobyov, E & Wiebe, D 2018, 'Chemical Signatures of the FU Ori Outbursts', Astrophysical Journal, vol. 866, no. 1, 46. https://doi.org/10.3847/1538-4357/aadfd9
Molyarova T, Akimkin V, Semenov D, Ábrahám P, Henning T, Kóspál A et al. Chemical Signatures of the FU Ori Outbursts. Astrophysical Journal. 2018 okt. 10;866(1). 46. https://doi.org/10.3847/1538-4357/aadfd9
Molyarova, Tamara ; Akimkin, Vitaly ; Semenov, Dmitry ; Ábrahám, P. ; Henning, Thomas ; Kóspál, Agnes ; Vorobyov, Eduard ; Wiebe, Dmitri. / Chemical Signatures of the FU Ori Outbursts. In: Astrophysical Journal. 2018 ; Vol. 866, No. 1.
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