activity
19972026
most citedThe X-ray emission from Nova V382 Velorum: II. The super-soft component observed with BeppoSAX

45 citations · 51 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026★ 1 cited

A comprehensive catalogue of high-mass X-ray binaries in the Large Magellanic Cloud detected during the first eROSITA all-sky survey

D. Kaltenbrunner, C. Maitra, F. Haberl +9

The Magellanic Clouds, the closest star-forming galaxies to the Milky Way, offer an excellent environment to study high-mass X-ray binaries. While the Small Magellanic Cloud has be…

astro-ph.SR2025★ 2 cited

The pre-eruption state of T CrB as observed with ALMA in 2024

D. Petry, G. Sala, I. El Mellah +2

T CrB is a nearby symbiotic binary and a recurrent nova with a period of ca. 80 years. The next eruption is expected to take place in 2025 or 2026. We present our pre-eruption obse…

astro-ph2002★ 45 cited

The X-ray emission from Nova V382 Velorum: II. The super-soft component observed with BeppoSAX

M. Orio, A. N. Parmar, J. Greiner +3

Nova Velorum 1999 (V382 Vel) was observed by BeppoSAX 6 months after optical maximum and was detected as a bright X-ray supersoft source, with a count rate 3.454+-0.002 cts/s in th…

astro-ph2001

Optical identification of supersoft X-ray sources in M31

Marina orio, Roberto Casalegno, Chris Conselice +3

We report on initial progress in a program of optical identification of supersoft X-ray sources in M31, pursued mainly with the WIYN telescope. We propose the identification of one…

astro-ph1997★ 3 cited

ROSAT Detection and High Precision Localization of X-ray Sources in the November 19, 1978 Gamma-Ray Burst Error Box

M. Boer, C. Motch, J. Greiner +3

We report on observations of the 1978, November 19 Gamma-Ray Burst source, performed with the ROSAT X-ray HRI experiment. Two sources were detected, one of which is possibly variab…