Rise and fall of the dust shell of the classical nova V339 Delphini
(2017)
Journal Article
We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a $\sim2$ year period. The infrared emission lines were initially symmetrical, with HWHM velocities of 525 km s$^{-1}$. In later ($t\gtrsim77$days, where $t$ is the t... Read More about Rise and fall of the dust shell of the classical nova V339 Delphini.