50 citations · 107 across the 4 of their papers we have counts for
5 papers
Two SMC Symbiotic stars undergoing steady hydrogen burning
M. orio, A. Zezas, U. Munari +2
Two symbiotic stars in the Small Magellanic Cloud (SMC), Lin 358 and SMC 3, have been supersoft X-ray sources (SSS) for more than 10 years. We fit atmospheric and nebular models to…
Variability and multi-periodic oscillations in the X-ray light curve of the classical nova V4743 Sgr
E. Leibowitz, M. Orio, R. Gonzalez-Riestra +5
The classical nova V4743 Sgr was observed with XMM-Newton for about 10 hours on April 4 2003, 6.5 months after optical maximum. At this time, this nova had become the brightest sup…
Chandra and XMM-Newton observations of the exceptional pulsar PSR B0628-28
E. Tepedelenlioglu, H. Ogelman
PSR B0628-28 is a radio pulsar which was first detected in the X-ray band by ROSAT and then later observed with Chandra and XMM-Newton. The Chandra observation yielded an X-ray lum…
Chandra observations of the recurrent nova IM Nor
Marina Orio, Emre Tepedelenlioglu, Sumner Starrfield +2
The recurrent nova IM Nor was observed twice in X-rays with Chandra ACIS-S, 1 and 6 months after the optical outburst. It was not detected in the first observation, with an upper l…
The Chandra Observations of the Two Pulsars PSR 0628-28 and PSR 1813-36
Hakki Ogelman, Emre Tepedelenlioglu
PSR B0628-28 is an X-ray emitting radio pulsar which was observed with Advanced CCD Imaging Spectrometer (ACIS) on board Chandra on 2001 November 04 and on 2002 March 25 for 2000 s…