activity
19962026
most citedThe Extraordinary X-ray Light Curve of the Classical Nova V1494 Aquilae (1999 #2) in Outburst: The Discovery of Pulsations and a "Burst"

69 citations · 544 across the 40 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

A very rapidly rotating white dwarf in nova YZ Reticuli

G. J. M. Luna, N. Rawat, R. Angeloni +4

YZ Ret (Nova Reticuli 2020) is the first VY Scl-type nova-like variable observed to undergo a classical nova eruption. Following the outburst, timing analysis of 20-s cadence TESS…

astro-ph.SR2018★ 18 cited

Optical observations of "hot" novae returning to quiescence

P. Zemko, S. Ciroi, M. Orio +10

We have monitored the return to quiescence of novae previously observed in outburst as supersoft X-ray sources, with optical photometry of the intermediate polar (IP) V4743 Sgr and…

astro-ph.SR2016★ 19 cited

V4743 Sgr, a magnetic nova?

P. Zemko, M. Orio, K. Mukai +3

Two XMM Newton observations of Nova V4743 Sgr (Nova Sgr 2002) were performed shortly after it returned to quiescence, 2 and 3.5 years after the explosion. The X-ray light curves re…

astro-ph.SR2016★ 25 cited

Pan-Chromatic observations of the Recurrent Nova LMC 2009a (LMC 1971b)

M. F. Bode, M. J. Darnley, A. P. Beardmore +11

Nova LMC 2009a is confirmed as a Recurrent Nova (RN) from positional coincidence with nova LMC 1971b. The observational data set is one of the most comprehensive for any Galactic o…

astro-ph.SR2015

Suzaku observation of the classical nova V2491 Cyg in quiescence

Polina Zemko, Koji Mukai, Marina Orio

We present Suzaku XIS observation of V2491 Cyg (Nova Cyg 2008 No. 2) obtained in quiescence, more than two years after the outburst. The nova was detected as a very luminous source…

astro-ph.SR2014★ 24 cited

X-ray observations of VY Scl type nova-like binaries in the high and low state

P. Zemko, M. Orio, K. Mukai +1

Four VY Scl-type nova-like systems were observed in X-rays during both the low and the high optical states. We examined Chandra, ROSAT, Swift and Suzaku archival observations of BZ…