activity
20082022
most citedThe nature and evolution of Nova Cygni 2006

29 citations · 40 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.SR20224 cited

The 2021 outburst of RS Oph: a pictorial atlas of the spectroscopic evolution. II. From day 19 to 102 (solar conjunction)

Ulisse Munari, Paolo Valisa

We present the second part (days 19 to 102) of our high-resolution Echelle atlas of the spectral evolution of RS Oph during the 2021 nova outburst. Some quick conclusions that can…

astro-ph.SR20216 cited

The 2021 outburst of RS Oph. A pictorial atlas of the spectroscopic evolution: the first 18 days

U. Munari, P. Valisa

A pictorial atlas of the spectroscopic evolution at optical wavelengths is presented for the first 18 days of the 2021 outburst of the recurrent nova RS Oph, prior to the emergence…

astro-ph.SR2021

The GALAH Survey and Symbiotic Stars. I. Discovery and follow-up of 33 candidate accreting-only systems

U. Munari, G. Traven, N. Masetti +14

We have identified a first group of 33 new candidates for symbiotic stars (SySt) of the accreting-only variety among the 600,255 stars so far observed by the GALAH high-resolution…

astro-ph.SR2020

Photometry and spectroscopy of the new symbiotic star 2SXPS J173508.4-292958

U. Munari, P. Valisa, A. Vagnozzi +3

We present and discuss the results of our photometric and spectroscopic monitoring of 2SXPS J173508.4-292958 carried out from April to August 2020. This X-ray source, in the foregr…

astro-ph.SR2019

The 2018 eruption and long term evolution of the new high-mass Herbig Ae/Be object Gaia-18azl = VES 263

U. Munari, V. Joshi, D. P. K. Banerjee +9

We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labeled as event Gaia-18azl. VES 2…

astro-ph.HE2019

Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560

Adrian B. Lucy, J. L. Sokoloski, U. Munari +11

How are accretion discs affected by their outflows? To address this question for white dwarfs accreting from cool giants, we performed optical, radio, X-ray, and ultraviolet observ…