activity
20122020
most citedX-ray observations of VY Scl type nova-like binaries in the high and low state

24 citations · 181 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2020★ 8 cited

X-ray Spectra and Light Curves of Cooling Novae and a Nova-Like

Bangzheng Sun, Marina Orio, Andrej Dobrotka +3

We present X-ray observations of novae V2491 Cyg and KT Eri about 9 years post-outburst, of the dwarf nova and post-nova candidate EY Cyg, and of a VY Scl variable. The first three…

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.HE2018★ 17 cited

What we learn from the X-ray grating spectra of Nova SMC 2016

M. Orio, J. -U. Ness, A. Dobrotka +17

Nova SMC 2016 has been the most luminous nova known in the direction of the Magellanic Clouds. It turned into a very luminous supersoft X-ray source between day 16 and 28 after the…

astro-ph.HE2017★ 16 cited

Constraining the accretion geometry of the intermediate polar EX Hya using NuSTAR, Swift and Chandra observations

G. J. M. Luna, K. Mukai, M. Orio +1

In magnetically accreting white dwarfs, the height above the white dwarf surface where the standing shock is formed is intimately related with the accretion rate and the white dwar…

astro-ph.HE2017★ 4 cited

CXO J004318.8+412016, a steady supersoft X-ray source in M 31

M. Orio, G. J. M. Luna, R. Kotulla +14

We obtained an optical spectrum of a star we identify as the optical counterpart of the M31 Chandra source CXO J004318.8+412016, because of prominent emission lines of the Balmer s…

astro-ph.SR2017★ 19 cited

Multi-mission observations of the old nova GK Per during the 2015 outburst

P. Zemko, M. Orio, G. J. M. Luna +3

GK Per, a classical nova of 1901, is thought to undergo variable mass accretion on to a magnetized white dwarf (WD) in an intermediate polar system (IP). We organized a multi-missi…