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T. Lanz

55 papers hereh-index 355.6k citations267 works total

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

author position
  • first author5
  • middle author35
  • last author10

Across the 50 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR26
  • astro-ph25
  • astro-ph.IM3
  • astro-ph.GA1
same name
  • T. Lanz — 5 papers, h 4
  • T. Lanz — 4 papers, h 4
  • T. Lanz — 1 paper, h 10
  • T. Lanz — 1 paper, h 20

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
19972022
most citedA Grid of NLTE Line-Blanketed Model Atmospheres of O-type Stars

741 citations · 3.5k across the 55 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 10 cited

Modeling multidimensional effects in the propagation of radiative shocks

Sébastien Leygnac, Laurent Boireau, Claire Michaut +4

Radiative shocks (also called supercritical shocks) are high Mach number shock waves that photoionize the medium ahead of the shock front and give rise to a radiative precursor. Th…

astro-ph2006★ 669 cited

A Grid of NLTE Line-Blanketed Model Atmospheres of Early B-type Stars

Thierry Lanz, Ivan Hubeny

We have constructed a comprehensive grid of 1540 metal line-blanketed, NLTE, plane-parallel, hydrostatic model atmospheres for the basic parameters appropriate to early B-type star…

astro-ph2006★ 16 cited

Iron in Hot DA White Dwarfs

Stephane Vennes, Pierre Chayer, Jean Dupuis +1

We present a study of the iron abundance pattern in hot hydrogen-rich (DA) white dwarfs. The study is based on new and archival far ultraviolet spectroscopy of a sample of white dw…

astro-ph2006★ 117 cited

Neon Abundances in B-Stars of the Orion Association: Solving the Solar Model Problem?

Katia Cunha, Ivan Hubeny, Thierry Lanz

We report on non-LTE Ne abundances for a sample of B-type stellar members of the Orion Association. The abundances were derived by means of non-LTE fully metal-blanketed model atmo…

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