activity
20082023
most citedGaia Photometric Science Alerts

134 citations · 830 across the 31 of their papers we have counts for

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Showing astro-ph.SRShow all

24 papers · 1 filter

astro-ph.SR2022★ 4 cited

Morpho-kinematic modeling of the expanding ejecta of the extremely slow nova V1280 Scorpii

Hiroyuki Naito, Akito Tajitsu, Valèrio A. R. M. Ribeiro +10

Morphology of nova ejecta is essential for fully understanding the physical processes involved in nova eruptions. We studied the 3D morphology of the expanding ejecta of the extrem…

astro-ph.SR2021

The 2019 outburst of the 2005 classical nova V1047 Cen: a record breaking dwarf nova outburst or a new phenomenon?

E. Aydi, K. V. Sokolovsky, J. S. Bright +28

We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years afte…

astro-ph.SR2020★ 14 cited

Radio light curves and imaging of the helium nova V445 Puppis reveal seven years of synchrotron emission

M. M. Nyamai, L. Chomiuk, V. A. R. M. Ribeiro +3

V445 Puppis is the only helium nova observed to date; its eruption in late 2000 showed high velocities up to 8500 km/s and a remarkable bipolar morphology cinched by an equatorial…

astro-ph.SR2019★ 16 cited

The January 2016 eruption of recurrent nova LMC 1968

N. P. M. Kuin, K. L. Page, P. Mróz +23

We present a comprehensive review of all observations of the eclipsing recurrent Nova LMC 1968 in the Large Magellanic Cloud which was previously observed in eruption in 1968, 1990…

astro-ph.SR2018★ 16 cited

The structure of a recent nova shell as observed by ALMA

Marcos P. Diaz, Zulema Abraham, Valério A. R. M. Ribeiro +2

High resolution ALMA observations of the recent (2.52 yrs old) shell of Nova V5668 Sgr (2015) show a highly structured ionised gas distribution with small (10 cm) clumps. Th…

astro-ph.SR2017★ 42 cited

A Recurrent Nova Super-Remnant in the Andromeda Galaxy

M. J. Darnley, R. Hounsell, T. J. O'Brien +11

Here we report that the most rapidly recurring nova, M31N 2008-12a, which erupts annually, is surrounded by a "nova super-remnant" which demonstrates that M31N 2008-12a has erupted…