activity
20082025
most citedThe nature and evolution of Nova Cygni 2006

29 citations · 88 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025★ 11 cited

T CrB: overview of the accretion history, Roche-lobe filling, orbital solution, and radiative modeling

U. Munari, F. Walter, N. Masetti +14

(abridged) We aim to derive a robust estimate of the most important parameters describing the physical nature of T CrB, trace the accretion history onto its white dwarf, and accoun…

astro-ph.SR2016★ 11 cited

The 2016 outburst of the unique symbiotic star MWC 560 (= V694 Mon), its long-term BVRI evolution and a marked 331 days periodicity

U. Munari, S. Dallaporta, F. Castellani +8

After 26 years from the major event of 1990, in early 2016 the puzzling symbiotic binary MWC 560 has gone into a new and even brighter outburst. We present our tight BVRI photometr…

astro-ph.SR2015★ 15 cited

500 days of Stromgren b, y and narrow-band [OIII], Ha photometric evolution of gamma-ray Nova Del 2013 (= V339 Del)

U. Munari, A. Maitan, S. Moretti +1

We present and discuss highly accurate photometry obtained through medium Stromgren y,b bands and narrow [OIII], Halpha bands covering 500 days of the evolution of Nova Del 2013 si…

astro-ph.SR2011★ 22 cited

Formation of a disk structure in the symbiotic binary AX Per during its 2007-10 precursor-type activity

A. Skopal, T. N. Tarasova, Z. Cariková +12

AX Per is an eclipsing symbiotic binary. During active phases, deep narrow minima are observed in its light curve, and the ionization structure in the binary changes significantly.…

astro-ph.SR2009

StHa 55: a carbon Mira, not a symbiotic binary

U. Munari, A. Siviero, M. Graziani +5

We carried out a VRI photometric monitoring of StHa 55, and in addition we obtained low resolution absolute spectro-photometry and high resolution Echelle spectroscopy. Our data sh…

astro-ph2008★ 29 cited

The nature and evolution of Nova Cygni 2006

U. Munari, A. Siviero, A. Henden +13

AIMS: Nova Cyg 2006 has been intensively observed throughout its full outburst. We investigate the energetics and evolution of the central source and of the expanding ejecta, their…