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researcher

W. Forman

39 papers hereh-index 447 citations23 works total

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

author position
  • middle author32
  • last author1

Across the 33 of 39 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO15
  • astro-ph.GA13
  • astro-ph.HE7
  • astro-ph3
  • astro-ph.IM1
same name
  • W. Forman — 258 papers, h 77
  • W. Forman — 44 papers, h 22
  • W. Forman — 39 papers, h 28
  • W. Forman — 13 papers
  • W. Forman — 11 papers, h 7
  • W. Forman — 5 papers, h 1

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
20002026
most citedGalaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey

708 citations · 3k across the 38 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2001★ 122 cited

Chandra Observation of RXJ1720.1+2638: a Nearly Relaxed Cluster with a Fast Moving Core?

P. Mazzotta, M. Markevitch, A. Vikhlinin +3

We have analyzed the Chandra observation of the distant (z=0.164) galaxy cluster RXJ1720.1+2638 in which we find sharp features in the X-ray surface brightness on opposite sides of…

astro-ph2000★ 313 cited

A High Resolution Study of the Hydra A Cluster with Chandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow

L. P. David, P. E. J. Nulsen, B. R. McNamara +5

The cooling flow cluster Hydra A was observed during the orbital activation and calibration phase of the Chandra Observatory. While the X-ray image of the cluster exhibits complex…

astro-ph2000★ 477 cited

Chandra Observation of Abell 2142: Survival of Dense Subcluster Cores in a Merger

M. Markevitch, T. J. Ponman, P. E. J. Nulsen +19

We use Chandra data to map the gas temperature in the central region of the merging cluster A2142. The cluster is markedly nonisothermal; it appears that the central cooling flow h…

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