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researcher

W. Forman

44 papers hereh-index 222k citations52 works total

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

author position
  • first author1
  • middle author32
  • last author4

Across the 37 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA13
  • astro-ph.HE13
  • astro-ph9
  • astro-ph.CO8
  • astro-ph.IM1
same name
  • W. Forman — 258 papers, h 77
  • W. Forman — 39 papers, h 28
  • W. Forman — 39 papers, h 4
  • 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
19972026
most citedAn investigation of cooling flows and general cluster properties from an X-ray image deprojection analysis of 207 clusters of galaxies

458 citations · 2.3k across the 43 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.CO2017★ 28 cited

Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra

I. Bartalucci, M. Arnaud, G. W. Pratt +6

We examine the reconstruction of galaxy cluster radial density profiles obtained from Chandra and XMM X-ray observations, using high quality data for a sample of twelve objects cov…

astro-ph.GA2017★ 40 cited

Galaxy-scale Bars in Late-type Sloan Digital Sky Survey Galaxies Do Not Influence the Average Accretion Rates of Supermassive Black Holes

Andy D. Goulding, Eve Matthaey, Jenny E. Greene +8

Galaxy-scale bars are expected to provide an effective means for driving material towards the central region in spiral galaxies, and possibly feeding supermassive black holes (BHs)…

astro-ph.GA2017★ 54 cited

Partitioning the Outburst Energy of a Low Eddington Accretion Rate AGN at the Center of an Elliptical Galaxy: the Recent 12 Myr History of the Supermassive Black Hole in M87

W. Forman, E. Churazov, C. Jones +3

M87, the active galaxy at the center of the Virgo cluster, is ideal for studying the interaction of a supermassive black hole (SMBH) with a hot, gas-rich environment. A deep Chandr…

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