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Table 1
Overview of proposed scenarios concerning the nature and the formation of the DSO/G2 and a few corresponding papers.
| Scenario | Papers |
|
|
|
| Murray-Clay & Loeb (2012), Eckart et al. (2013), Scoville & Burkert (2013), Ballone et al. (2013) | |
| Star with dusty envelope/disc and outflow | Zajaček et al. (2014), De Colle et al. (2014), Valencia-S. et al. (2015), Ballone et al. (2016), Shahzamanian et al. (2016) |
|
|
|
| Binary/binary dynamics | Zajaček et al. (2014), Prodan et al. (2015), Witzel et al. (2014), Stephan et al. (2016) |
|
|
|
| Gillessen et al. (2012), Burkert et al. (2012), Schartmann et al. (2012), Shcherbakov (2014) | |
| Core-less cloud/streamer | Pfuhl et al. (2015), Schartmann et al. (2015), McCourt et al. (2015), McCourt & Madigan (2016), Madigan et al. (2017) |
|
|
|
| Tidal disruption | Miralda-Escudé (2012), Guillochon et al. (2014) |
|
|
|
| Nova outburst | Meyer & Meyer-Hofmeister (2012) |
|
|
|
| Planet/protoplanet | Mapelli & Ripamonti (2015), Trani et al. (2016) |
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