activity
19922024
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 9.6k across the 232 of their papers we have counts for

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Showing 1995 · astro-phShow all

7 papers · 2 filters

astro-ph1995

The missing x-rays in Sgr A*: evidence for - not against - a supermassive black hole

Heino Falcke, Peter L. Biermann

We present a simple argument that the missing x-ray flux from the Galactic Center source Sgr~A* ist not evidence {\it against} -- as claimed by Goldwurm et al. 1994 -- but rather i…

astro-ph1995

ROSAT PSPC observations of six PG quasars and PHL 1657

Joerg P. Rachen, Karl Mannheim, Peter L. Biermann

We report results from the spectral analysis of pointed ROSAT PSPC observations of six PG quasars and the weak-bump quasar PHL 1657. Disregarding other frequency bands, the PSPC da…

astro-ph1995★ 10 cited

Galactic jet sources and the AGN connection

Heino Falcke, Peter L. Biermann

In order to further test our hypothesis that jets and disk around compact accreting objects are symbiotic features we investigate the newly discovered superluminal galactic radio j…

astro-ph1995

SUPERNOVA BLASTWAVES AND PRE-SUPERNOVA WINDS: THEIR COSMIC RAY CONTRIBUTION

Peter L. Biermann

Supernova explosions into predecessor stellar winds can lead to particle acceleration, which we suggest can explain most of the observed cosmic rays of the nuclei of Helium and hea…

astro-ph1995★ 18 cited

The origin of cosmic rays

Peter L. Biermann

The search for the origin of cosmic rays is a quest of almost a hundred years. A recent theoretical proposal gives quantitative predictions, which can be tested with data. Specific…

astro-ph1995

THE ORIGIN OF COSMIC RAYS

Peter L. Biermann

We propose that cosmic rays originate mainly in three sites, a) normal supernova explosions into the interstellar medium, b) supernova explosions into stellar winds, and c) hot spo…

astro-ph1995★ 44 cited

The Origin of Galactic Cosmic Rays

Peter L. Biermann, T. K. Gaisser, Todor Stanev

Motivated by recent measurements of the major components of the cosmic radiation around 10 TeV/nucleon and above, we discuss the phenomenology of a model in which there are two dis…