Guo, Z;
Lucas, PW;
Kurtev, R;
Borissova, J;
Peña, CC;
Yurchenko, SN;
Smith, LC;
... Muthu, HDS; + view all
(2024)
Spectroscopic confirmation of high-amplitude eruptive YSOs and dipping giants from the VVV survey.
Monthly Notices of the Royal Astronomical Society
, 528
(2)
pp. 1769-1788.
10.1093/mnras/stad3700.
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Abstract
During the pre-main-sequence (pre-MS) evolution stage of a star, significant amounts of stellar mass are accreted during episodic accretion events, such as multidecade FUor-type outbursts. Here, we present a near-infrared spectroscopic follow-up study of 33 high-amplitude (most with ΔKs > 4 mag) variable sources discovered by the Vista Variables in the Via Lactea (VVV) survey. Based on the spectral features, 25 sources are classified as eruptive young stellar objects (YSOs), including 15 newly identified FUors, six with long-lasting, but EXor-like bursts of magnetospheric accretion and four displaying outflow-dominated spectra. By examining the photometric behaviours of eruptive YSOs, we found most FUor-type outbursts have higher amplitudes (ΔKs and ΔW2), faster eruptive time-scales and bluer infrared colours than the other outburst types. In addition, we identified seven post-MS variables apparently associated with deep dipping events and an eruptive star with deep aluminium monoxide absorption bands resembling those seen in the V838 Mon stellar merger.
Type: | Article |
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Title: | Spectroscopic confirmation of high-amplitude eruptive YSOs and dipping giants from the VVV survey |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1093/mnras/stad3700 |
Publisher version: | http://dx.doi.org/10.1093/mnras/stad3700 |
Language: | English |
Additional information: | This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third-party material in this article are included in the Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
Keywords: | Stars: AGB and post-AGB, stars: pre-main-sequence, stars: protostar, stars: variables: T Tauri, Herbig Ae/Be, infrared: stars |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/10187512 |
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