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P. Salom'e

41 papers hereh-index 201.1k citations42 works total

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

author position
  • first author4
  • middle author27
  • last author6

Across the 37 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.CO7
  • astro-ph4
same name
  • P. Salom'e — 8 papers, h 2
  • P. Salom'e — 8 papers, h 3

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
20042026
most citedUbiquitous cold and massive filaments in cool core clusters

154 citations · 1.6k across the 41 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 20 cited

Search for cold gas along radio lobes in the cooling core galaxies MS0735.6+7421 and M87

P. Salomé, F. Combes

We report CO observations towards MS0735.6+7421 a distant cooling core galaxy, and towards M87, the nearest cooling core in the center of the Virgo cluster. Both galaxies contain r…

astro-ph2008★ 42 cited

Observations of CO in the eastern filaments of NGC 1275

P. Salomé, Y. Revaz, F. Combes +4

We recently found extended CO(2-1) emission from cold molecular gas embedded in the network of Halpha filaments surrounding the galaxy NGC 1275 (Salome et al. 2006). We now present…

astro-ph2006

CO(2-1) large scale mapping of the Perseus cluster core with HERA

Philippe Salomé, Francoise Combes

Cold molecular gas has recently been found is several cooling flow clusters cores with single dish telescopes. High spatial resolution imaging of some of these clusters then reveal…

astro-ph2004★ 18 cited

Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared?

P. Schuller, P. Salomé, G. Perrin +7

Recently available near-infrared interferometric data on late-type stars show a strong increase of diameter for asymptotic giant branch (AGB) stars between the K (2.0 - 2.4 μm) and…

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