activity
20042007
most citedXMM-Newton observations of the first unidentified TeV gamma-ray source TeV J2032+4130

24 citations · 26 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2007★ 24 cited

XMM-Newton observations of the first unidentified TeV gamma-ray source TeV J2032+4130

D. Horns, A. I. D. Hoffmann, A. Santangelo +2

(abridged) The first unidentified very high energy gamma ray source (TeV J2032+4130) in the Cygnus region has been the subject of intensive search for a counterpart source at other…

astro-ph2005

X-RED: A Satellite Mission Concept To Detect Early Universe Gamma Ray Bursts

Mirko Krumpe, Deirdre Coffey, Georg Egger +14

Gamma ray bursts (GRBs) are the most energetic eruptions known in the Universe. Instruments such as Compton-GRO/BATSE and the GRB monitor on BeppoSAX have detected more than 2700 G…

astro-ph2005

Light and heavy metal abundances in hot central stars of planetary nebulae

K. Werner, A. I. D. Hoffmann, D. Jahn +5

We present new results from our spectral analyses of very hot central stars achieved since the last IAU Symposium on planetary nebulae held in Canberra 2001. The analyses are mainl…

astro-ph2004

Iron Abundance in Hydrogen-Rich Central Stars of Planetary Nebulae

A. I. D. Hoffmann, I. Traulsen, T. Rauch +3

We report on an on-going analysis of high-resolution UV spectra of hot hydrogen-rich central stars of planetary nebulae (CSPN), obtained with the Hubble Space Telescope and FUSE. S…

astro-ph2004★ 2 cited

HST and FUSE Spectroscopy of Hot Hydrogen-Rich Central Stars of Planetary Nebulae

I. Traulsen, A. I. D. Hoffmann, T. Rauch +3

High-resolution UV spectra, obtained with HST and FUSE, enable us to analyse hot hydrogen-rich central stars in detail. Up to now, optical hydrogen and helium lines have been used…