papers

Publications (22)

astro-ph.SR2014

Study of three 2013 novae: V1830 Aql, V556 Ser and V809 Cep

U. Munari, P. Ochner, S. Dallaporta +7

BVRI photometry and low-, medium- and high-resolution Echelle fluxed spectroscopy is presented and discussed for three faint, heavily reddened novae of the FeII-type which erupted…

astro-ph.SR2011

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.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.SR2023

Atlas of photometric and spectroscopic daily monitoring of the very slow Nova Cas 2021 (=V1405 Cas) during the first 660 days of its outburst

P. Valisa, U. Munari, S. Dallaporta +2

Nova Cas 2021 erupted on 18 March 2021, reaching naked-eye brightness when passing through photometric maximum 53 days later. We describe our ~daily monitoring of its evolution, co…

astro-ph.HE2022

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…