activity
20172022
most citedProlonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

38 citations · 49 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20223 cited

Transient behavior of three SU UMa-type dwarf novae; AR Pic, QW Ser and V521 Peg

Hélène Szegedi, Philip A. Charles, Pieter J. Meintjes +1

Changes in the supercycle lengths of some SU UMa-type dwarf novae have been detected by other studies, and indicate that the mass transfer rates noticeably decrease over time. We i…

astro-ph.HE201938 cited

Prolonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

Francesco Coti Zelati, Alessandro Papitto, Domitilla de Martino +12

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim…

astro-ph.SR2018

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.HE20174 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.HE20174 cited

An eLIMA model for the 67 s X-ray periodicity in CAL 83

A. Odendaal, P. J. Meintjes

Supersoft X-ray sources (SSSs) are characterized by their low effective temperatures and high X-ray luminosities. The soft X-ray emission can be explained by hydrogen nuclear burni…