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R. Kraft

29 papers hereh-index 467.9k citations414 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author15
  • last author2

Across the 22 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph23
  • astro-ph.CO4
  • astro-ph.HE2
same name
  • R. Kraft — 4 papers, h 16
  • R. Kraft — 1 paper, h 3
  • R. Kraft — 1 paper, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20032011
most citedHigh-energy particle acceleration at the radio-lobe shock of Centaurus A

147 citations · 729 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

4 papers · 1 filter

astro-ph.CO2011★ 54 cited

Markarian 6: shocking the environment of an intermediate Seyfert

Beatriz Mingo, Martin J. Hardcastle, Judith H. Croston +4

Markarian 6 is a nearby (D~78 Mpc) Seyfert 1.5, early-type galaxy, with a double set of radio bubbles. The outer set spans ~7.5 kpc and is expanding into the halo regions of the ho…

astro-ph.CO2011

ICM Signatures from Multiple Outbursts in the Galaxy Group NGC 5813: A Window to AGN Feedback

S. W. Randall, W. R. Forman, S. Giacintucci +10

We present results from Chandra observations of NGC 5813, the dominant central galaxy in a nearby galaxy group. We focus on three main results. 1) The diffuse gas shows clear signa…

astro-ph.CO2009

Suzaku Observations of the Radio Galaxy 3C 33

Daniel A. Evans, James N. Reeves, Martin J. Hardcastle +3

We present results from a new 100-ks Suzaku observation of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. W…

astro-ph.CO2009★ 1 cited

Nature of X-shaped sources

D. V. Lal, M. J. Hardcastle, R. P. Kraft +5

The nature of X-shaped sources is a matter of considerable debate: it has even been proposed that they provide evidence for black hole mergers/spin reorientation, and therefore…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.