University of Hertfordshire

From the same journal

From the same journal

By the same authors

Documents

  • 2103-13335v1

    Accepted author manuscript, 5.36 MB, PDF document

  • Zhen Guo
  • P. W. Lucas
  • Carlos Contreras Pena
  • L. C. Smith
  • C. Morris
  • R. G. Kurtev
  • J. Borissova
  • J. Alonso-García
  • D. Minniti
  • A. -N. Chené
  • M. S. N. Kumar
  • A. Caratti o Garatti
  • D. Froebrich
View graph of relations
Original languageEnglish
Article numberstab882
Number of pages28
JournalMonthly Notices of the Royal Astronomical Society
Early online date26 Mar 2021
DOIs
Publication statusE-pub ahead of print - 26 Mar 2021

Abstract

The decade-long Vista Variables in the Via Lactea (VVV) survey has detected numerous highly variable young stellar objects (YSOs). We present a study of 61 highly variable VVV YSOs (Delta Ks = 1-5 mag), combining near infrared spectra from Magellan and VLT with VVV and NEOWISE light curves to investigate physical mechanisms behind eruptive events. Most sources are spectroscopically confirmed as eruptive variables (typically Class I YSOs) but variable extinction is also seen. Among them, magnetically controlled accretion, identified by HI recombination emission (usually accompanied by CO emission), is observed in 46 YSOs. Boundary layer accretion, associated with FU Ori-like outbursts identified by CO overtone and H2O absorption, is observed only in longer duration events (>=5 yr total duration). However, even in long duration events, the magnetically controlled accretion mode predominates, with amplitudes similar to the boundary layer mode. Shorter (100-700 days) eruptive events usually have lower amplitudes and these events are generally either periodic accretors or multiple timescale events, wherein large photometric changes occur on timescales of weeks and years. We find that the ratio of amplitudes in Ks and W2 can distinguish between variable accretion and variable extinction. Several YSOs are periodic or quasi-periodic variables. We identify examples of periodic accretors and extinction-driven periodicity among them (with periods up to 5 yr) though more data are needed to classify some cases. The data suggest that dynamic interactions with a companion may control the accretion rate in a substantial proportion of eruptive systems, although star-disc interactions should also be considered.

Notes

© 2021 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stab882

ID: 24917306