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researcher

Sébastien Peirani

4 papers here

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

author position
  • first author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.GA1
ORCID 0000-0001-6902-2898

identity via Semantic Scholar / OpenAlex

activity
20072009
most citedA giant bar induced by a merger event at z=0.4?

48 citations · 124 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2009★ 42 cited

A forming, dust enshrouded disk at z=0.43: the first example of a late type disk rebuilt after a major merger?

F. Hammer, H. Flores, Y. B. Yang +4

Abreg: By combining HST/UDF imagery with kinematics from VLT/GIRAFFE we derive a physical model of distant galaxy J033245.11-274724.0 in a way similar to what can be done in the ne…

astro-ph2008★ 48 cited

A giant bar induced by a merger event at z=0.4?

Sébastien Peirani, Francois Hammer, Hector Flores +2

(Aims) We present a physical model of the formation of J033239.72-275154.7, a galaxy observed at z=0.41 and characterized by a big young bar of size 6 kpc. The study of this system…

astro-ph2008★ 33 cited

Dark Matter Accretion into Supermassive Black Holes

Sébastien Peirani, José Antonio De Freitas Pacheco

The relativistic accretion rate of dark matter by a black hole is revisited. Under the assumption that the phase space density indicator, Q=ρ∞​/σ∞3​, remains const…

astro-ph2007★ 1 cited

Phase-Space Evolution of Dark Matter Halos

S. Peirani, J. A. de Freitas Pacheco

(Context) In a Universe dominated by dark matter, halos are continuously accreting mass (violently or not) and such mechanism affects their dynamical state. (Aims) The evolution of…

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