› Forums › Spectroscopy › ASASSN-19de (TCP J06373299-0935420) › Identity
23 February 2019 at 6:17 pm
#580739
![](https://britastro.org/wp-content/uploads/2021/02/picture-7761-1614033711-80x80.jpg)
Participant
Hi Robin. Very interesting. Am I right in thinking this would be consistent with an accretion disk in an optically thick state? Or are there other – perhaps more likely – explanations?