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Multiple flares caused by mass ejection episodes during the advanced nebular phase of Nova Scuti 2019
U. Munari, G. L. Righetti, S. Dallaporta
Our photometric and spectroscopic monitoring shows that starting with 2020 June 4, day +217 from optical maximum and well into its advanced nebular stage, Nova Sct 2019 began displ…
Persistent nuclear burning in Nova Sgr 2016 N.4 (= V5856 Sgr = ASASSN-16ma) six years past its outburst
U. Munari, N. Masetti, F. M. Walter +4
We report on the fast Nova Sgr 2016 N.4 being surprisingly trapped in a long-lasting and bright plateau (Delta I >= 10 mag above quiescence) six years past the nova eruption. Very…
GIARPS High-resolution Observations of T Tauri stars (GHOsT). IV. Accretion properties of the Taurus-Auriga young association
M. Gangi, S. Antoniucci, K. Biazzo +9
In the framework of the GIARPS@TNG High-resolution Observations of T Tauri stars (GHOsT) project, we study the accretion properties of 37 Classical T Tauri Stars of the Taurus-Auri…
Stringent limits on SiO maser emission from the recurrent nova T Coronae Borealis
A. Evans, B. Pimpanuwat, A. M. S. Richards +5
There are indications that the third known eruption of the recurrent nova T CrB is imminent, and multi-wavelength observations prior to the eruption are important to characterise t…